The modified Einstein field equations of f(T) gravity with a clear analogy to GR equations are given by [31,32,33]
$$\begin{aligned} f'G_{ab}+\frac{1}{2} g_{ab} [f-f'T]-f''S_{ab}^{~~~c}\nabla _c T = \kappa ^2\mathscr {T}^{}_{ab}, \end{aligned}$$
(1)
where \(f' \equiv df/dT\), \(f''\equiv d^2f/dT^2\), \(\mathscr {T} _{ab}\) denotes the usual EMT of the matter fluid expressed as
$$\begin{aligned}&\mathscr {T} ^b_{a} = \frac{1}{e}\frac{\delta ( e L_m)}{\delta e^{b}_{a}}, \end{aligned}$$
(2)
and the coupling constant \(\kappa ^2\equiv \frac{8\pi G}{c^4}\). The above field equations can be re-written in a more compact form as
$$\begin{aligned} G_{ab} = \mathscr {T}^{T}_{ab} +\mathscr {T}^{(m)}_{ab}, \end{aligned}$$
(3)
where we have defined the EMT of the torsion (T) fluid as [31]
$$\begin{aligned} \mathscr {T}^T_{ab}= & {} -\frac{1}{2f'}g_{ab} (f-f'T)-\frac{1}{f'}(f''S_{ab}^{~~d}\nabla _d T) \nonumber \\&-\frac{1}{f'}(f'-1)\mathscr {T}^{(m)}_{ab}. \end{aligned}$$
(4)
In the limiting case of \(f(T) = T\) (cf. [31, 32]) the field equations reduce to those of GR.Footnote 1 From this generalized form of the gravitational field equations of motion in f(T) gravity, we obtain the modified Friedmann and Raychaudhuri equations in f(T) for FLRW spacetimes as followsFootnote 2:
$$\begin{aligned}&H^2= \frac{\rho _m}{3f'} -\frac{1}{6f'}(f-Tf'), \end{aligned}$$
(5)
$$\begin{aligned}&2\dot{H} + 3H^2 = \frac{p_{m}}{f'} +\frac{1}{2f'}(f-Tf')+ \frac{4f''H\dot{T}}{f'}, \end{aligned}$$
(6)
where H(t) is the Hubble (expansion) parameter defined from the scale factor a(t) and the cosmic time t as \(H\equiv \frac{\dot{a}}{a}\). One can compute the torsion contributions of the thermodynamical quantities such as energy density \(\rho _T\) and pressure \(p_T\) from the EMT of the torsion fluid as follows:
$$\begin{aligned}&\rho _T = -\frac{1}{f'}\left[ (f'-1)\rho _m +\frac{1}{2}(f-Tf')\right] , \end{aligned}$$
(7)
$$\begin{aligned}&p_T = -\frac{1}{f'}\left[ (f'-1)p_m -\frac{1}{2}(f-Tf')\right] +2H\frac{f''}{f'}\dot{T},\nonumber \\ \end{aligned}$$
(8)
where \(\rho _m\) is the energy density, \(p_m\) is the pressure of the matter fluid, torsion scalar \( T = -6H^2\). Here we assume a slowly changing torsion fluid i.e., \(\dot{T}\approx 0\) such that the pressure of the torsion fluid is given by
$$\begin{aligned} p_T = -\frac{1}{f'}\left[ (f'-1)p_m -\frac{1}{2}(f-Tf')\right] . \end{aligned}$$
(9)
Since the effective energy density of the fluid \(\rho _{eff}\) is the sum of the two non-interacting fluid components (matter and torsion), we have the effective (total) energy density
$$\begin{aligned} \rho _{eff} \equiv \rho _m +\rho _T, \end{aligned}$$
(10)
and the effective pressure of the total fluid is
$$\begin{aligned} p_{eff} \equiv p_m +p_T. \end{aligned}$$
(11)
Then, the corresponding conservation equation of the fluid is
$$\begin{aligned}&\dot{\rho } \equiv -3H\left( \rho _{eff} +p_{eff}\right) . \end{aligned}$$
(12)
From the modified Friedmann equation (5), the effective energy density of the total fluid is
$$\begin{aligned} \rho _{eff} = \frac{\rho _m}{f'} - \frac{1}{2f'} \left( f-Tf'\right) , \end{aligned}$$
(13)
and the corresponding effective pressure takes the form
$$\begin{aligned} p_{eff} = \frac{p_m}{f'} +\frac{1}{2f'}(f-Tf'). \end{aligned}$$
(14)
In the special case \(f(T) = T\), Eqs. (1)–(14) all reduce to the GR limit, which in turn describes similar cosmic dynamics as GR. A cosmological fluid of particular interest in recent years is the so-called CG. It is a fluid model proposed as a candidate for a unified description of dark matter and dark energy [4, 29, 34], and its cosmological scenarios are widely presented in the literature. In this work, we consider the torsion fluid as an exotic fluid with equations of state similar to the ones for three variants of the CG model and we reconstruct f(T) gravity toy models corresponding to the original, generalized and modified generalized models. The characteristic equation of state for the CG model is given by [4, 35]
$$\begin{aligned} p=-\frac{A}{\rho ^{\alpha }}, \end{aligned}$$
(15)
where \(0<\alpha \le 1\), A is a positive constant and the energy density \(\rho >0\).
Now, if we consider the possibility of the torsion fluid mimicking the CG with the characteristic equation of state given by
$$\begin{aligned} p_T=-\frac{A}{\rho _T^{\alpha }}, \end{aligned}$$
(16)
and substitute the energy density \(\rho _T\) and pressure \(p_T\) of the torsion fluid from Eqs. (7) and (9) into Eq. (16), we obtain the master equation
$$\begin{aligned}&-\frac{1}{f'}\left[ (f'-1)p_m -\frac{1}{2}(f-Tf')\right] \nonumber \\&\quad \bigg [-\frac{1}{f'}\left( (f'-1)\rho _m +\frac{1}{2}(f-Tf')\right) \bigg ]^\alpha =-A, \end{aligned}$$
(17)
from which our solution process starts. This is a general expression of the equation of state to reconstruct different f(T) gravity models from the given two paradigmatic models of CG (original and generalized) and in the following two sections we reconstruct different f(T) gravity models based on Eq. (17). As a consequence of field equation (1) and the EMT of the torsion fluid Eq. (4), the Lagrangian density of f(T) gravity for different systems may depend on the torsion and matter fluids. A similar way of f(T) representation is done in [36].
Let us discuss the scheme that we follow in the original and generalized CG models. We first reconstruct the f(T) gravity model for five different cases: vacuum, radiation-torsion, dust-torsion, stiff matter-torsion and radiation-dust-torsion systems for both CG models. Then, secondly, we substitute the reconstructed f(T) gravity models into Eqs. (7) and (9) and compute the corresponding energy density, pressure and the equation of state parameter of the torsion fluid for each case in these CG models. The energy density of each fluid apart from that of CG is expressed as
$$\begin{aligned}&\rho _d = \rho _{d0}a^{-3}, \\&\rho _r = \rho _{r0}a^{-4}, ~~\text{ and } \\&\rho _s =\rho _{s0}a^{-6}, \end{aligned}$$
where \(\rho _d\), \(\rho _r\) and \(\rho _s\) are the energy density for dust, radiation and stiff matter fluids respectively and \(\rho _{i0}\) denotes the present-day value of the energy density of fluid type \(i=\{d, r ,s\}\).Footnote 3 Consequently, we compute the effective energy density and pressure of the effective fluid as well, the equation of state parameter for torsion fluid \(w_T\) and we present the numerical plots of the effective equation state parameters \(w_{eff(j)}\) for all total fluids as
$$\begin{aligned} w_{eff(j)} = \frac{p^j_T+p^i}{\rho _T^j+\rho ^i}, \end{aligned}$$
(18)
where the indice \(j\equiv \{1, 2 ,3,\ldots N\}\) depends on the number of reconstructed f(T) gravity solutions, because we have more than one reconstructed f(T) gravity models for each CG model. Thirdly, we define the parameter \(\xi _j\) to represent the growth factor of the energy densities of the torsion fluid as
$$\begin{aligned} \xi _j = \frac{\rho ^j_T}{\rho ^j_{T0}}, \end{aligned}$$
(19)
where \(\rho _{T0}\) represents the energy density of the torsion in the present day. We also define another dimensionless parameter \(\chi _j\) to represent the fraction of the effective energy densities of the total fluid from Eq. (10) as
$$\begin{aligned} \chi _j = \frac{\rho _{eff(j)}}{\rho _{eff0(j)}}, \end{aligned}$$
(20)
where \(\rho _{eff0}\) denotes the energy density of the total fluid in the present day for radiation-torsion, dust-torsion and radiation-dust-torsion systems in each CG model. Then, we present the numerical plots of \(\xi \) and \(\chi \) versus the scale factor a for radiation-torsion, dust-torsion and radiation-dust-torsion systems. This is the set of procedures we follow to reconstruct different f(T) gravity models and the corresponding thermodynamic quantities accordingly. Similar procedures apply for the MGCG model, the only difference being the modified equation of state Eq. (168) we will use instead of Eq. (17). Finally, we have put a generalized discuss for all evolution of the equation of state parameters and the fractional energy densities in Sect. (4).
2.1 Reconstructing modified teleparallel gravity from the OCG model
In the OCG model, the equation of state Eq. (15) has \(\alpha =1\) [24, 39], and with the torsion fluid acting as the exotic CG fluid, we will have
$$\begin{aligned} p_T=-\frac{A}{\rho _T}. \end{aligned}$$
(21)
In the following, different f(T)-gravity models will be reconstructed for vacuum, radiation-torsion, dust-torsion, stiff matter-torsion and radiation-dust-torsion systems in the OCG model.
2.1.1 Vacuum system
In this case we assume the energy density and the pressure of the matter fluid are negligible, \(\rho _m = p_m=0\) and that torsion manifests itself as a CG. From the general expression of Eq. (17), we obtain
$$\begin{aligned} \left( T^2-4A\right) f'^2-2fTf'+f^2=0, \end{aligned}$$
(22)
thus obtaining two possible f(T) gravity models as solutions:
$$\begin{aligned}&f_1(T)= c\left( T - 2\sqrt{A} \right) , \end{aligned}$$
(23)
$$\begin{aligned}&f_2(T)= c\left( T + 2\sqrt{A} \right) , \end{aligned}$$
(24)
where \(c \ne 0\) and it is an integration constant. By substituting \(f_1(T)\) and \(f_2(T)\) into Eq. (7), the energy density of the torsion fluid becomes
$$\begin{aligned} \rho _T = \pm \sqrt{A}. \end{aligned}$$
(25)
As we indicated earlier in Eq. (15), the energy density of this exotic fluid is always positive and different from zero. Then, we take only the positive term of Eq. (25) \(\rho _T = \sqrt{A}\), resulting in a negative pressure. This energy density agrees with the result in [34]. Consequently, we only take the negative term from the reconstructed f(T) gravity, \(f(T)= cT - 2c\sqrt{A},\) such that \( p_T = -{\sqrt{A}},\) and the equation of state parameter of the torsion fluid \( w_T = {p_T}/{\rho _T} = -1\). In the case of \(f(T) = T\), the f(T) gravity theory coincides with GR. Here, we observe that the obtained equation of state parameter of torsion asymptotically approaches the DE phase \(w = -1\). This indicates that the torsion fluid acts as an exotic fluid and it is an alternative approach to describe the accelerated expansion of the Universe.
2.1.2 Radiation-torsion system
Here we reconstruct torsion-radiation coupling by considering a non-interacting two-component fluid system of the Universe such that Eq. (17) is given as
$$\begin{aligned}&-\frac{1}{f'}\left[ (f'-1)\frac{1}{3}\rho _r -\frac{1}{2}(f-Tf')\right] \nonumber \\&\quad \bigg [-\frac{1}{f'}\left( (f'-1)\rho _r +\frac{1}{2}(f-Tf')\right) \bigg ]=-A\;. \end{aligned}$$
(26)
From this equation we obtain four different f(T) gravity models as follows:
$$\begin{aligned} f_1 \left( T \right)= & {} T{ c}-2/3\rho _r\,{ c}+2/3\rho _r + 2/3\, \sqrt{4\,{{ c}}^{2}{\rho _r}^{2}+9\,A{{ c}}^{2}-8{ c }\,{\rho _r}^{2}+4\,{\rho _r}^{2}}, \end{aligned}$$
(27)
$$\begin{aligned} f_2\left( T \right)= & {} T{ c}-2/3\,\rho _r\,{ c}-2/3\;, \rho _r + 2/3\, \sqrt{4\,{{ c}}^{2}{\rho _r}^{2}+9\,A{{ c}}^{2}-8, { c }\,{\rho _r}^{2}+4\,{\rho _r}^{2}}, \end{aligned}$$
(28)
$$\begin{aligned} f_3\left( T \right)= & {} 2\,{\frac{ \left( 2\,T\rho _r+3\,A+\sqrt{-9\,A{T}^{ 2}+12\,AT\rho _r+12\,A{\rho _r}^{2}+36\,{A}^{2}} \right) \rho _r}{4 {\rho _r}^{2} +9\,A}}, \end{aligned}$$
(29)
$$\begin{aligned} f_4 \left( T \right)= & {} 2\,{\frac{ \left( 2\,T\rho _r+3\,A-\sqrt{-9\,A{T}^{ 2}+12\,AT\rho _r+12\,A{\rho _r}^{2}+36\,{A}^{2}} \right) \rho _r}{4 {\rho _r}^{2} +9\,A}}. \end{aligned}$$
(30)
In some limiting cases, where \(\rho _r = 0\), \( f_1(T)\) and \(f_2(T)\) in Eqs. (27) and (28) are reduced to the vacuum system in Eqs. (23) and (24) respectively, while other f(T) gravity models such as \( f_3(T)\) and \( f_4(T)\) in Eqs. (29) and (30) go to zero. By substituting Eqs. (27)–(30) into Eq. (7), we bring in the corresponding energy density of the torsion fluid as follows:
$$\begin{aligned}&\rho ^1_T = \,{\frac{-2\,\rho _r\,{ c}+2\,\rho _r+\sqrt{4\, \left( { c} -1 \right) ^{2}{\rho _r}^{2}+9\,A{{ c}}^{2}}}{3{ c}}}\;, \end{aligned}$$
(31)
$$\begin{aligned}&\rho ^2_T = 1/3\,{\frac{-2\,\rho _r\,{ c}+2\,\rho _r-\sqrt{4\, \left( { c} -1 \right) ^{2}{\rho _r}^{2}+9\,A{{ c}}^{2}}}{{ c}}} \;, \end{aligned}$$
(32)
$$\begin{aligned}&\rho _T^3 = -3\,{\frac{ \left( \left( \frac{2}{3}\,\rho _r\,T-\frac{4}{3}\,{\rho _r}^{2}-2\,A \right) \sqrt{3}+\sqrt{A \left( -3\,{T}^{2}+4\,\rho _r\,T+4\,{\rho _r}^{2} +12\,A \right) } \right) A}{3\,\sqrt{3}A \left( T-2/3\,\rho _r \right) -2\, \rho _r\,\sqrt{A \left( -3\,{T}^{2}+4\,\rho _r\,T+4\,{\rho _r}^{2}+12\,A \right) }}} \;, \end{aligned}$$
(33)
$$\begin{aligned}&\rho _T^4 = 3\,{\frac{A \left( \left( -2/3\,\rho _r\,T+4/3\,{\rho _r}^{2}+2\,A \right) \sqrt{3}+\sqrt{A \left( -3\,{T}^{2}+4\,\rho _r\,T+4\, {\rho _r}^{2 }+12\,A \right) } \right) }{2\,\rho _r\,\sqrt{A \left( -3\,{T}^{2} +4\, \rho _r\,T+4\,{\rho _r}^{2}+12\,A \right) }+3\,\sqrt{3}A \left( T-2/3\,\rho _r \right) }}\;. \end{aligned}$$
(34)
In a similar manner, we present the corresponding pressure of the torsion fluid in the era of radiation by substituting Eqs. (27)–(30) into Eq. (9). So, the reconstructed pressures of the torsion fluid are given as follows:
$$\begin{aligned}&p^1_T = \,{\frac{-4\,\rho _r\,{ c}+4\,\rho _r-\sqrt{4\, \left( { c} -1 \right) ^{2}{\rho _r}^{2}+9\,A{{ c}}^{2}}}{3{ c}}}, \end{aligned}$$
(35)
$$\begin{aligned}&p^{2}_{T} = 1/3\,{\frac{-4\,\rho _r\,{ c}+4\,\rho _r+\sqrt{4\, \left( { c} -1 \right) ^{2}{\rho _r}^{2}+9\,A{{ c}}^{2}}}{{ c}}}, \end{aligned}$$
(36)
$$\begin{aligned}&p_T^3 = -6\,{\frac{A \left( -\sqrt{A \left( -3\,{T}^{2}+4\,\rho _r\,T+4\, {\rho _r} ^{2}+12\,A \right) }+\sqrt{3} \left( 2/3\,\rho _r\,T+A \right) \right) }{2\,\rho _r\,\sqrt{A \left( -3\,{T}^{2}+4\,\rho _r\,T+4\,{\rho _r}^{2} +12\,A \right) }+3\,\sqrt{3}A \left( T-2/3\,\rho _r \right) }}, \end{aligned}$$
(37)
$$\begin{aligned}&p^4_T = -6\,{\frac{A \left( \sqrt{A \left( -3\,{T}^{2}+4\,\rho _r\,T+4\, {\rho _r}^ {2}+12\,A \right) }+\sqrt{3} \left( 2/3\,\rho _r\,T+A \right) \right) }{-2\,\rho _r\,\sqrt{A \left( -3\,{T}^{2}+4\,\rho _r\,T+4\,{\rho _r}^{2} +12\,A \right) }+3\,\sqrt{3}A \left( T-2/3\,\rho _r \right) }}. \end{aligned}$$
(38)
Therefore from Eqs. (31)–(34) and Eqs. (35)–(38) we also present the equation of state parameters of the torsion fluid accordingly:
$$\begin{aligned}&w^1_T = {\frac{-4\,\rho _r\,{ c}+4\,\rho _r-\sqrt{4\, \left( { c}-1 \right) ^{2}{\rho _r}^{2}+9\,A{{ c}}^{2}}}{-2\,\rho _r\,{ c}+2 \,\rho _r+\sqrt{4\, \left( { c}-1 \right) ^{2}{\rho _r}^{2}+9\, A{{ c}}^{2}}}}, \end{aligned}$$
(39)
$$\begin{aligned}&w^{2}_{T} = {\frac{4\,\rho _r\,{ c}-\sqrt{4\, \left( { c}-1 \right) ^{2 }{\rho _r}^{2}+9\,A{{ c}}^{2}}-4\,\rho _r}{2\,\rho _r\,{ c}+ \sqrt{ 4\, \left( { c}-1 \right) ^{2}{\rho _r}^{2}+9\,A{{ c}}^ {2}}-2 \,\rho _r}}, \end{aligned}$$
(40)
$$\begin{aligned}&w_T^3 = {\frac{6\,\sqrt{A \left( -3\,{T}^{2}+4\,\rho _r\,T+4\,{\rho _r}^{2} +12\,A \right) }+ \left( -4\,\rho _r\,T-6\,A \right) \sqrt{3}}{3\,\sqrt{A \left( -3\,{T}^{2}+4\,\rho _r\,T+4\,{\rho _r}^{2}+12\,A \right) }+ \left( - 2\,\rho _r\,T+4\,{\rho _r}^{2}+6\,A \right) \sqrt{3}}}, \end{aligned}$$
(41)
$$\begin{aligned}&w_T^4 = {\frac{-6\,\sqrt{A \left( -3\,{T}^{2}+4\,\rho _r\,T+4\,{\rho _r}^{2} +12\,A \right) }+ \left( -4\,\rho _r\,T-6\,A \right) \sqrt{3}}{-3\,\sqrt{A \left( -3\,{T}^{2}+4\,\rho _r\,T+4\,{\rho _r}^{2}+12\,A \right) }+ \left( - 2\,\rho _r\,T+4\,{\rho _r}^{2}+6\,A \right) \sqrt{3}}}. \end{aligned}$$
(42)
We apply the definition of Eq. (18) and we represent the numerical plots of the equation of state parameter for the radiation-torsion system in the following figure for OCG Fig. 1.Footnote 4
Then, the growth factor of the energy density of the torsion fluid in the radiation dominated era from the above thermodynamic quantities become:
$$\begin{aligned} \xi _1 = \frac{\rho ^1_{T}}{\rho ^1_{T_0}}\;, \qquad \xi _2 = \frac{\rho ^2_{T}}{\rho ^2_{T_0}} \;, \qquad \xi _3 = \frac{\rho ^3_{T}}{\rho ^3_{T_0}}\;, \qquad \xi _4 = \frac{\rho ^4_{T}}{\rho ^4_{T_0}}.\nonumber \\ \end{aligned}$$
(43)
And from Eqs. (31)–(34), we obtain the growth factor of the energy density for effective fluid as follows:
$$\begin{aligned}&\xi _1 = \,{\frac{-2\,\rho _r\,{ c}+2\,\rho _r+\sqrt{4\, \left( { c} -1 \right) ^{2}{\rho _r}^{2}+9\,A{{ c}}^{2}}}{\,{{-2\,\rho _{r,0}\,{ c}+2\,\rho _{r,0}+\sqrt{4\, \left( { c} -1 \right) ^{2}{\rho _{r,0}}^{2}+9\,A{{ c}}^{2}}}}}} \;, \end{aligned}$$
(44)
$$\begin{aligned}&\xi _2 = \frac{{ \,{-2\,\rho _r\,{ c}+2\,\rho _r-\sqrt{4\, \left( { c} -1 \right) ^{2}{\rho _r}^{2}+9\,A{{ c}}^{2}}}}{}}{{\,{-2\,\rho _{r,0}\,{ c}+2\,\rho _{r,0}-\sqrt{4\, \left( { c} -1 \right) ^{2}{\rho _{r,0}}^{2}+9\,A{{ c}}^{2}}}}{}}\;, \end{aligned}$$
(45)
$$\begin{aligned}&\xi _3 = \frac{-3\,{\frac{ \left( \left( 2/3\,\rho _r\,T-4/3\,{\rho _r}^{2}-2\,A \right) \sqrt{3}+\sqrt{A \left( -3\,{T}^{2}+4\,\rho _r\,T+4\,{\rho _r}^{2} +12\,A \right) } \right) A}{3\,\sqrt{3}A \left( T-2/3\,\rho _r \right) -2\, \rho _r\,\sqrt{A \left( -3\,{T}^{2}+4\,\rho _r\,T+4\,{\rho _r}^{2}+12\,A \right) }}}}{-3\,{\frac{ \left( \left( 2/3\,\rho _{r,0}\,T-4/3\,{\rho _{r,0}}^{2}-2\,A \right) \sqrt{3}+\sqrt{A \left( -3\,{T}^{2}+4\,\rho _{r,0}\,T+4\,{\rho _{r,0}}^{2} +12\,A \right) } \right) A}{3\,\sqrt{3}A \left( T-2/3\,\rho _{r,0} \right) -2\, \rho _{r,0}\,\sqrt{A \left( -3\,{T}^{2}+4\,\rho _{r,0}\,T+4\,{\rho _{r,0}}^{2}+12\,A \right) }}}}\;,\nonumber \\ \end{aligned}$$
(46)
$$\begin{aligned}&\xi _4 = \frac{-3\,{\frac{ \left( \left( 2/3\,\rho _r\,T-4/3\,{\rho _r}^{2}-2\,A \right) \sqrt{3}-\sqrt{A \left( -3\,{T}^{2}+4\,\rho _r\,T+4\,{\rho _r}^{2} +12\,A \right) } \right) A}{3\,\sqrt{3}A \left( T-2/3\,\rho _r \right) +2\, \rho _r\,\sqrt{A \left( -3\,{T}^{2}+4\,\rho _r\,T+4\,{\rho _r}^{2}+12\,A \right) }}}}{-3\,{\frac{ \left( \left( 2/3\,\rho _{r,0}\,T-4/3\,{\rho _{r,0}}^{2}-2\,A \right) \sqrt{3}-\sqrt{A \left( -3\,{T}^{2}+4\,\rho _{r,0}\,T+4\,{\rho _{r,0}}^{2} +12\,A \right) } \right) A}{3\,\sqrt{3}A \left( T-2/3\,\rho _{r,0} \right) +2\, \rho _{r,0}\,\sqrt{A \left( -3\,{T}^{2}+4\,\rho _{r,0}\,T+4\,{\rho _{r,0}}^{2}+12\,A \right) }}}} \;.\nonumber \\ \end{aligned}$$
(47)
Here we also present the other dimensionless parameter \(\chi \) to represent the fraction of the effective energy density of the radiation-torsion fluid:
$$\begin{aligned} \begin{aligned}&\chi _1 = \frac{\rho ^1_{eff}}{\rho ^1_{eff_0}},\qquad \chi _2 = \frac{\rho ^2_{eff}}{\rho ^2_{eff_0}}\;, \\&\chi _1 = \frac{\rho ^3_{eff}}{\rho ^3_{eff_0}}\;, \qquad \chi _4 = \frac{\rho ^4_{eff}}{\rho ^4_{eff_0}}\;, \end{aligned} \end{aligned}$$
(48)
the explicit values of which are given by:
$$\begin{aligned}&\chi _1 = \frac{3c\rho _r +{ \,{-2\,\rho _r\,{ c}+2\,\rho _r+\sqrt{4\, \left( { c} -1 \right) ^{2}{\rho _r}^{2}+9\,A{{ c}}^{2}}}}{}}{ 3c\rho _{r,0}+{\,{-2\,\rho _{r,0}\,{ c}+2\,\rho _{r,0}+\sqrt{4\, \left( { c} -1 \right) ^{2}{\rho _{r,0}}^{2}+9\,A{{ c}}^{2}}}}{}}\;, \end{aligned}$$
(49)
$$\begin{aligned}&\chi _2 = \frac{3c\rho _r +{ \,{-2\,\rho _r\,{ c}+2\,\rho _r-\sqrt{4\, \left( { c} -1 \right) ^{2}{\rho _r}^{2}+9\,A{{ c}}^{2}}}}{}}{ 3c\rho _{r,0}+{\,{-2\,\rho _{r,0}\,{ c}+2\,\rho _{r,0}-\sqrt{4\, \left( { c} -1 \right) ^{2}{\rho _{r,0}}^{2}+9\,A{{ c}}^{2}}}}{}}\;, \end{aligned}$$
(50)
$$\begin{aligned}&\chi _3 = \frac{\rho _r -3\,{\frac{ \left( \left( 2/3\,\rho \,T-4/3\,{\rho _r}^{2}-2\,A \right) \sqrt{3}+\sqrt{A \left( -3\,{T}^{2}+4\,\rho _r\,T+4\,{\rho _r}^{2} +12\,A \right) } \right) A}{3\,\sqrt{3}A \left( T-2/3\,\rho _r \right) -2\, \rho _r\,\sqrt{A \left( -3\,{T}^{2}+4\,\rho _r\,T+4\,{\rho _r}^{2}+12\,A \right) }}}}{\rho _{r,0}-3\,{\frac{ \left( \left( 2/3\,\rho _{r,0}\,T-4/3\,{\rho _{r,0}}^{2}-2\,A \right) \sqrt{3}+\sqrt{A \left( -3\,{T}^{2}+4\,\rho _{r,0}\,T+4\,{\rho _{r,0}}^{2} +12\,A \right) } \right) A}{3\,\sqrt{3}A \left( T-2/3\,\rho _{r,0} \right) -2\, \rho _{r,0}\,\sqrt{A \left( -3\,{T}^{2}+4\,\rho _{r,0}\,T+4\,{\rho _{r,0}}^{2}+12\,A \right) }}}}\;,\nonumber \\ \end{aligned}$$
(51)
$$\begin{aligned}&\chi _4 = \frac{\rho _r -3\,{\frac{ \left( \left( 2/3\,\rho _r\,T-4/3\,{\rho _r}^{2}-2\,A \right) \sqrt{3}-\sqrt{A \left( -3\,{T}^{2}+4\,\rho _r\,T+4\,{\rho _r}^{2} +12\,A \right) } \right) A}{3\,\sqrt{3}A \left( T-2/3\,\rho _r \right) +2\, \rho _r\,\sqrt{A \left( -3\,{T}^{2}+4\,\rho _r\,T+4\,{\rho _r}^{2}+12\,A \right) }}}}{\rho _{r,0}-3\,{\frac{ \left( \left( 2/3\,\rho _{r,0}\,T-4/3\,{\rho _{r,0}}^{2}-2\,A \right) \sqrt{3}-\sqrt{A \left( -3\,{T}^{2}+4\,\rho _{r,0}\,T+4\,{\rho _{r,0}}^{2} +12\,A \right) } \right) A}{3\,\sqrt{3}A \left( T-2/3\,\rho _{r,0} \right) +2\, \rho _{r,0}\,\sqrt{A \left( -3\,{T}^{2}+4\,\rho _{r,0}\,T+4\,{\rho _{r,0}}^{2}+12\,A \right) }}}}.\nonumber \\ \end{aligned}$$
(52)
All the above thermodynamic quantities namely \(\rho _T\), \(p_T\), \(w_T\) and \(\rho _{eff}\) are depend on the energy density of the radiation fluid \(\rho _r\) and \(\rho _r\) is proportional to the cosmological scale factor. Consequently, the energy density parameters such as \(\xi \) and \(\chi \) also depend the scale factor of the Universe. One can obtain the growth factor of the energy densities of the fluids \(\xi \) and \(\chi \); here we present numerical results in Fig. 2.
2.1.3 Dust-torsion system
After the era of radiation, the Universe was predominantly filled by pressureless matter ( dust) fluid. Thus, in a dust-dominated Universe, \(p_d \approx 0\), and the equation of state parameter is \(w_d \approx 0\). In our current model, we consider the non-interacting dust-torsion system and briefly discuss its implications for cosmic expansion. The general expression of Eq. (17) in the dust-torsion system becomes
$$\begin{aligned} \frac{1}{{f'}^{2}}\left[ \frac{1}{4}(f-Tf')^{2}+\frac{1}{2}(f'-1)(f-Tf') \rho _d\right] =A\;,\quad \end{aligned}$$
(53)
and this equation admits four different f(T) gravity models as solutions:
$$\begin{aligned}&f_1(T) = (1-c)\rho _d +cT + \sqrt{(c^{2}-2c)\rho _d^2 +4c^{2}_1 A }\;, \end{aligned}$$
(54)
$$\begin{aligned}&f_2(T) = (1-c)\rho _d +cT - \sqrt{(c^{2}-2c)\rho _d^2 +4c^{2}_1 A }\;, \end{aligned}$$
(55)
$$\begin{aligned}&f_3(T) = \frac{\rho _d}{\rho _d^2+4A}\left[ \rho _d T+4A-2\sqrt{-AT^2+2AT\rho _d+4A^2}\right] \;,\nonumber \\ \end{aligned}$$
(56)
$$\begin{aligned}&f_4(T) = \frac{\rho _d}{\rho _d^2+4A}\left[ \rho _d T+4A+2\sqrt{-AT^2+2AT\rho _d+4A^2}\right] .\nonumber \\ \end{aligned}$$
(57)
For \(\rho _d = 0\), two of the solutions, Eqs. (54) and (55), reduce to the vacuum case, Eqs. (23) and (24) respectively, whereas the other two solutions, Eqs. (56) and (57), vanish. Let us now substitute \( f_1(T)\), \( f_2(T)\), \( f_3(T)\) and \( f_4(T)\) into Eqs. (7) and (9) to obtain the energy densities of the torsion
$$\begin{aligned}&\rho ^1_T = \,{\frac{-\rho _d\,{ c}+\rho _d+\sqrt{ \left( { c}-1 \right) ^{2}{\rho _d}^{2}+4\,A{{ c}}^{2}}}{2{ c}}} \;, \end{aligned}$$
(58)
$$\begin{aligned}&\rho ^{T}_{2} = \,{\frac{-\rho _d\,{ c}+\rho _d-\sqrt{ \left( { c}-1\right) ^{2}{\rho _d}^{2}+4\,A{{ c}}^{2}}}{2{ c}}}\;, \end{aligned}$$
(59)
$$\begin{aligned}&\rho _T^3 = {\frac{A \left( -\rho _d\,T+2\,{\rho _d}^{2}+4\,A+2\,\sqrt{4\,{A}^ {2}-T \left( T-2\,\rho _d \right) A} \right) }{\rho _d\,\sqrt{4\,{A}^{2}-T \left( T-2\,\rho _d \right) A}+2\,A \left( T-\rho _d \right) }}\;,\nonumber \\ \end{aligned}$$
(60)
$$\begin{aligned}&\rho _T^4 = {\frac{A \left( -T\rho _d+2\,{\rho _d}^{2}+2\,A - \sqrt{A \left( -{T}^ {2}+4 \,{\rho _d}^{2}+4\,A \right) } \right) }{AT+\rho _d\,\sqrt{A \left( - {T}^{2 }+4\,{\rho _d}^{2}+4\,A \right) }}}\;,\nonumber \\ \end{aligned}$$
(61)
and the corresponding isotropic pressures
$$\begin{aligned}&p^1_T = \,{\frac{-3\,\rho _d\,{ c}+3\,\rho _d-\sqrt{ \left( { c}-1 \right) ^{2}{\rho _d}^{2}+4\,A{{ c}}^{2}}}{2{ c}}}\;, \end{aligned}$$
(62)
$$\begin{aligned}&p_{T}^{2} = \,{\frac{-3\,{ c}\,\rho _d+3\,\rho _d+\sqrt{ \left( { c}-1 \right) ^{2}{\rho _d}^{2}+4\,A{{ c}}^{2}}}{2{ c}}}\;, \end{aligned}$$
(63)
$$\begin{aligned}&p_T^3 = {\frac{A \left( -3\,\rho _d\,T+2\,{\rho _d}^{2}+6\,\sqrt{4\,{A}^{2}- T \left( T-2\,\rho _d \right) A}4A \right) }{ \left( 2\,T-2\,\rho _d \right) A+\rho _d\,\sqrt{4\,{A}^{2}-T \left( T-2\,\rho _d \right) A} }}\;,\nonumber \\ \end{aligned}$$
(64)
$$\begin{aligned}&p_T^4 = -{\frac{A \left( T\rho _d+2\,{\rho _d}^{2}+2\,A-\sqrt{A \left( -{T}^{2}+4 \,{\rho _d}^{2}+4\,A \right) } \right) }{AT+\rho _d\,\sqrt{A \left( - {T}^{2 }+4\,{\rho _d}^{2}+4\,A \right) }}}\;.\nonumber \\ \end{aligned}$$
(65)
The reconstructed EoS parameters of the torsion fluid during the dust-dominated phase \(w_T = p_T/\rho _T\) are then given by:
$$\begin{aligned}&w_T^1 = {\frac{-3\,\rho _d\,{ c}+3\,\rho _d-\sqrt{ \left( { c}-1 \right) ^{2}{\rho _d}^{2}+4\,A{{ c}}^{2}}}{-\rho _d\,{ c} +\rho _d+ \sqrt{ \left( { c}-1 \right) ^{2}{\rho _d}^{2}+4\,A{{ c}}^{2 }}}}\;, \end{aligned}$$
(66)
$$\begin{aligned}&w_{T}^{2}= {\frac{3\,{ c}\,\rho _d-\sqrt{ \left( { c}-1 \right) ^{2}{ \rho _d}^{2}+4\,A{{ c}}^{2}}-3\,\rho _d}{{ c}\,\rho _d+\sqrt{ \left( { c}-1 \right) ^{2}{\rho _d}^{2}+4\,A{{ c}}^{2} }-\rho _d}}\;, \end{aligned}$$
(67)
$$\begin{aligned}&w_T^3 = {\frac{-3\,\rho _d\,T+2\,{\rho _d}^{2}+6\,\sqrt{4\,{A}^{2}-T \left( T-2\, \rho _d \right) A}4A}{-\rho _d\,T+2\,{\rho _d}^{2}+4\,A+2\,\sqrt{4\, {A}^{2} -T \left( T-2\,\rho _d \right) A}}}\;,\nonumber \\ \end{aligned}$$
(68)
$$\begin{aligned}&w_T^4 = {\frac{-T\rho _d-2\,{\rho _d}^{2}-2\,A+\sqrt{A \left( -{T}^{2}+4\, {\rho _d}^{ 2}+4\,A \right) }}{-T\rho _d+2\,{\rho _d}^{2}+2\,A+\sqrt{A \left( - {T}^{2}+ 4\,{\rho _d}^{2}+4\,A \right) }}}.\nonumber \\ \end{aligned}$$
(69)
We use Eq. (18) and represent the numerical plots of the equation of state parameter for the dust-torsion system in Fig. 3 figure for OCG.
Moreover, the fractional energy densities of torsion in the dust-torsion system give as follows:
$$\begin{aligned}&\xi _1 = \,\frac{-\rho _d\,{ c}+\rho _d+\sqrt{ \left( { c}-1 \right) ^{2}{\rho _d}^{2}+4\,A{{ c}}^{2}}}{-\rho _{d,0}\,{ c}+\rho _{d,0}+\sqrt{ \left( { c}-1 \right) ^{2}{\rho _{d,0}}^{2}+4\,A{{ c}}^{2}}} \;, \end{aligned}$$
(70)
$$\begin{aligned}&\xi _2 = \frac{\,{ {-\rho _d\,{ c}+\rho _d-\sqrt{ \left( { c}-1\right) ^{2}{\rho _d}^{2}+4\,A{{ c}}^{2}}}{}}}{\,{{-\rho _{d,0}\,{ c}+\rho _{d,0}-\sqrt{ \left( { c}-1\right) ^{2}{\rho _{d,0}}^{2}+4\,A{{ c}}^{2}}}{}}} \;, \end{aligned}$$
(71)
$$\begin{aligned}&\xi _3 = \frac{{\frac{A \left( -\rho \,T+2\,{\rho }^{2}+4\,A+2\,\sqrt{4\,{A}^ {2}-T \left( T-2\,\rho \right) A} \right) }{\rho \,\sqrt{4\,{A}^{2}-T \left( T-2\,\rho \right) A}+2\,A \left( T-\rho \right) }}}{{\frac{A \left( -\rho _{d,0}\,T+2\,{\rho _{d,0}}^{2}+4\,A+2\,\sqrt{4\,{A}^ {2}-T \left( T-2\,\rho _{d,0}\right) A} \right) }{\rho _{d,0}\,\sqrt{4\,{A}^{2}-T \left( T-2\,\rho _{d,0} \right) A}+2\,A \left( T-\rho _{d,0} \right) }}} \;, \end{aligned}$$
(72)
$$\begin{aligned}&\xi _4 = \frac{{\frac{A \left( -T\rho +2\,{\rho }^{2}+2\,A - \sqrt{A \left( -{T}^ {2}+4 \,{\rho }^{2}+4\,A \right) } \right) }{AT+\rho \,\sqrt{A \left( - {T}^{2 }+4\,{\rho }^{2}+4\,A \right) }}}}{ {\frac{A \left( -T\rho _{d,0}+2\,{\rho _{d,0}}^{2}+2\,A - \sqrt{A \left( -{T}^ {2}+4 \,{\rho _{d,0}}^{2}+4\,A \right) } \right) }{AT+\rho _{d,0}\,\sqrt{A \left( - {T}^{2 }+4\,{\rho _{d,0}}^{2}+4\,A \right) }}}}\;, \end{aligned}$$
(73)
and for the effective fluid, these become:
$$\begin{aligned}&\chi _1 = \,\frac{\rho _d\,{ c}+\rho _d+\sqrt{ \left( { c}-1 \right) ^{2}{\rho _d}^{2}+4\,A{{ c}}^{2}}}{\rho _{d,0}\,{ c}+\rho _{d,0}+\sqrt{ \left( { c}-1 \right) ^{2}{\rho _{d,0}}^{2}+4\,A{{ c}}^{2}}} \;, \end{aligned}$$
(74)
$$\begin{aligned}&\chi _2 = \,\frac{\rho _d\,{ c}+\rho _d-\sqrt{ \left( { c}-1 \right) ^{2}{\rho _d}^{2}+4\,A{{ c}}^{2}}}{\rho _{d,0}\,{ c}+\rho _{d,0}-\sqrt{ \left( { c}-1 \right) ^{2}{\rho _{d,0}}^{2}+4\,A{{ c}}^{2}}} \;, \end{aligned}$$
(75)
$$\begin{aligned}&\chi _3 = \frac{{\rho _d + \frac{A \left( -\rho \,T+2\,{\rho }^{2}+4\,A+2\,\sqrt{4\,{A}^ {2}-T \left( T-2\,\rho \right) A} \right) }{\rho \,\sqrt{4\,{A}^{2}-T \left( T-2\,\rho \right) A}+2\,A \left( T-\rho \right) }}}{\rho _{d,0} + {\frac{A \left( -\rho _{d,0}\,T+2\,{\rho _{d,0}}^{2}+4\,A+2\,\sqrt{4\,{A}^ {2}-T \left( T-2\,\rho _{d,0}\right) A} \right) }{\rho _{d,0}\,\sqrt{4\,{A}^{2}-T \left( T-2\,\rho _{d,0} \right) A}+2\,A \left( T-\rho _{d,0} \right) }}} \;,\nonumber \\ \end{aligned}$$
(76)
$$\begin{aligned}&\chi _4 = \frac{\rho _d+{\frac{A \left( -T\rho +2\,{\rho }^{2}+2\,A - \sqrt{A \left( -{T}^ {2}+4 \,{\rho }^{2}+4\,A \right) } \right) }{AT+\rho \,\sqrt{A \left( - {T}^{2 }+4\,{\rho }^{2}+4\,A \right) }}}}{\rho _{d,0} +{\frac{A \left( -T\rho _{d,0}+2\,{\rho _{d,0}}^{2}+2\,A - \sqrt{A \left( -{T}^ {2}+4 \,{\rho _{d,0}}^{2}+4\,A \right) } \right) }{AT+\rho _{d,0}\,\sqrt{A \left( - {T}^{2 }+4\,{\rho _{d,0}}^{2}+4\,A \right) }}}} \;.\nonumber \\ \end{aligned}$$
(77)
In Fig. 4, we present the growth of the fractional energy densities for torsion and effective fluids versus the scale factor.
2.1.4 Stiff matter-torsion system
Here, we consider a Universe composed of stiff matter ( \(p_s=\rho _s\) with \(w=1\)) and torsion. The general expression of Eq. (17) for such a system is given as
$$\begin{aligned}&-\frac{1}{f'}\left[ (f'-1)\rho _s -\frac{1}{2}(f-Tf')\right] \nonumber \\&\quad \bigg [-\frac{1}{f'}\left( (f'-1)\rho _s +\frac{1}{2}(f-Tf')\right) \bigg ]=-A. \end{aligned}$$
(78)
From this expression we reconstruct four different f(T) gravity models as follows:
$$\begin{aligned}&f_1 \left( T \right) =T{ c}-2\,\sqrt{{{ c}}^{2} {\rho _s}^{2}+A {{ c}}^{2}-2\,{ c}\,{\rho _s}^{2}+{\rho _s}^{2}}\;, \end{aligned}$$
(79)
$$\begin{aligned}&f_2\left( T \right) =T{ c}+2\,\sqrt{{{ c}}^{2} {\rho _s}^{2}+A {{ c}}^{2}-2\,{ c}\,{\rho _s}^{2}+{\rho _s}^{2}}\;, \end{aligned}$$
(80)
$$\begin{aligned}&f_3\left( T \right) ={\frac{ \left( T\rho _s+\sqrt{-A{T}^{2}+4\,A {\rho _s}^ {2}+4\,{A}^{2}} \right) \rho _s}{{\rho _s}^{2}+A}}\;, \end{aligned}$$
(81)
$$\begin{aligned}&f_4 \left( T \right) =-{\frac{ \left( -T\rho _s+\sqrt{-A{T}^{2} +4\,A{\rho _s }^{2}+4\,{A}^{2}} \right) \rho _s}{{\rho _s}^{2}+A}}.\nonumber \\ \end{aligned}$$
(82)
Here also we see that setting \(\rho _s = 0\) reduces two of the f(T) gravity models, Eqs. (79) and (80), to the vacuum cases, Eqs. (23) and (24) we studied earlier, whereas the other two solutions, Eqs. (81) and (82), both vanish. By substituting the above f(T) solutions into Eq. (7), we obtain the corresponding energy densities and isotropic pressures of the torsion fluid in the era of stiff matter as follows:
$$\begin{aligned}&\rho ^1_T= {\frac{-\rho _s\,{ c}+\rho _s+\sqrt{ \left( { c}-1 \right) ^{2 }{\rho _s}^{2}+A{{ c}}^{2}}}{{ c}}} \;, \end{aligned}$$
(83)
$$\begin{aligned}&\rho ^2_T = {\frac{-\rho _s\,{ c}+\rho _s-\sqrt{ \left( { c}-1 \right) ^{2}{\rho _s}^{2}+A{{ c}}^{2}}}{{ c}}} \;, \end{aligned}$$
(84)
$$\begin{aligned}&\rho _T^3 = {\frac{A \left( -T\rho _s+2\,{\rho _s}^{2}+2\,A-\sqrt{A \left( -{T}^ {2}+4\,{\rho _s}^{2}+4\,A \right) } \right) }{AT-\rho _s\,\sqrt{A \left( - {T}^{2 }+4\,{\rho _s}^{2}+4\,A \right) }}}\;,\nonumber \\ \end{aligned}$$
(85)
$$\begin{aligned}&\rho ^4_T = {\frac{A \left( -T\rho _s+2\,{\rho _s}^{2}+2\,A+\sqrt{A \left( -{T}^ {2}+4 \,{\rho _s}^{2}+4\,A \right) } \right) }{AT+\rho _s\,\sqrt{A \left( - {T}^{2 }+4\,{\rho _s}^{2}+4\,A \right) }}}\;,\nonumber \\ \end{aligned}$$
(86)
$$\begin{aligned}&p_T^1 = {\frac{-\rho _s\,{ c}+\rho _s-\sqrt{ \left( { c}-1 \right) ^{2 }{\rho _s}^{2}+A{{ c}}^{2}}}{{ c}}}\;, \end{aligned}$$
(87)
$$\begin{aligned}&p_T^2 = {\frac{-{ c}\,\rho _s+\rho _s+\sqrt{ \left( { c}-1 \right) ^{2 }{\rho _s}^{2}+A{{ c}}^{2}}}{{ c}}}\;, \end{aligned}$$
(88)
$$\begin{aligned}&p_T^3 = -{\frac{A \left( T\rho _s+2\,{\rho _s}^{2}+2\,A+\sqrt{A \left( -{T}^ {2}+4 \,{\rho _s}^{2}+4\,A \right) } \right) }{AT-\rho _s\,\sqrt{A \left( - {T}^{2 }+4\,{\rho _s}^{2}+4\,A \right) }}}\;,\nonumber \\ \end{aligned}$$
(89)
$$\begin{aligned}&p_T^4 = -{\frac{A \left( T\rho _s+2\,{\rho _s}^{2}+2\,A-\sqrt{A \left( -{T}^ {2}+4 \,{\rho _s}^{2}+4\,A \right) } \right) }{AT+\rho _s\,\sqrt{A \left( - {T}^{2 }+4\,{\rho _s}^{2}+4\,A \right) }}}\;.\nonumber \\ \end{aligned}$$
(90)
We also compute the equation of state parameter of the torsion fluid in the stiff fluid-torsion system as follows:
$$\begin{aligned}&w_T^1 = {\frac{-\rho _s\,{ c}+\rho _s-\sqrt{ \left( { c}-1 \right) ^{2 }{\rho _s}^{2}+A{{ c}}^{2}}}{-\rho _s\,{ c}+\rho _s+\sqrt{ \left( { c}-1 \right) ^{2}{\rho _s}^{2}+A{{ c}}^{2}}}}\;, \end{aligned}$$
(91)
$$\begin{aligned}&w_T^2 = {\frac{{ c}\,\rho _s-\sqrt{ \left( { c}-1 \right) ^ {2}{\rho _s }^{2}+A{{ c}}^{2}}-\rho _s}{{ c}\,\rho _s+\sqrt{ \left( { c}-1 \right) ^{2}{\rho _s}^{2}+A{{ c}}^{2}}-\rho _s}} \;, \end{aligned}$$
(92)
$$\begin{aligned}&w_T^3 = \frac{-T\rho _s-2\,{\rho _s}^{2}-2\,A-\sqrt{A \left( -{T}^{2}+4\, {\rho _s}^{ 2}+4\,A \right) }}{-T\rho _s+2\,{\rho _s}^{2}+2\,A-\sqrt{A \left( - {T}^{2}+ 4\,{\rho _s}^{2}+4\,A \right) }}\;,\nonumber \\ \end{aligned}$$
(93)
$$\begin{aligned}&w_T^4 = {\frac{-T\rho _s-2\,{\rho _s}^{2}-2\,A+\sqrt{A \left( -{T}^{2}+4\, {\rho _s}^{ 2}+4\,A \right) }}{-T\rho _s+2\,{\rho _s}^{2}+2\,A+\sqrt{A \left( - {T}^{2}+ 4\,{\rho _s}^{2}+4\,A \right) }}}.\nonumber \\ \end{aligned}$$
(94)
2.1.5 Radiation-dust-torsion system
Here, we consider a non-interacting multi-fluid system, namely radiation and dust with torsion, and those fluids acts as an exotic fluid for cosmic expansion. In this context, all thermodynamical quantities are the mixture of the individual species. For instance, the pressure of the effective fluid is given as \( p_{eff} = p_m +p_T.\) The general form of Eq. (17) for radiation-dust-torsion system is given as
$$\begin{aligned}&-\frac{1}{f'}\left[ (f'-1)p -\frac{1}{2}(f-Tf')\right] \nonumber \\&\quad \bigg [-\frac{1}{f'}\left( (f'-1)\rho +\frac{1}{2}(f-Tf')\right) \bigg ]=-A\;, \end{aligned}$$
(95)
where the energy density of matter \(\rho = \rho _r + \rho _d\). We reconstruct four different f(T) gravity models through this system as follows:
$$\begin{aligned}&f_1 \left( T \right) =-{ c}\,{ \rho _d}+T{ c}-2/3\,{ c}\,\rho _r+{ \rho _d}+2/3\,\rho _r \nonumber \\&\quad - 1/3 \bigg [9\,{{ \rho _d}}^{2}{{ c}}^{2}+24\,{{ c}}^{2}{ \rho _d}\,\rho _r+16\,{{ c}}^{2} {\rho _r}^{2}\nonumber \\&\quad +36\,A{{ c}}^{2}-18\,{{ \rho _d}}^{2}{ c}-48\,{ c}\,{ \rho _d}\,\rho _r-32\,{ c}\,{\rho _r}^{2}\nonumber \\&\quad +9\,{{ \rho _d}}^{2} +24\,{ \rho _d}\,\rho _r+16\,{\rho _r}^{2}\bigg ]\;, \end{aligned}$$
(96)
$$\begin{aligned}&f_2 \left( T \right) =-{ c}\,{ \rho _d}+T{ c}-2/3\,{ c} \,\rho _r+{ \rho _d}+2/3\,\rho _r \nonumber \\&\quad +1/3 \bigg [9\,{{ \rho _d}}^{2}{{ c}}^ {2}+24\,{{ c}}^{2}{ \rho _d}\,\rho _r +16\,{{ c}}^{2} {\rho _r}^{2}\nonumber \\&\quad +36\,A{{ c}}^{2}-18\,{{ \rho _d}}^{2}{ c}-48\,{ c}\,{ \rho _d}\,\rho _r-32\,{ c}\,{\rho _r}^{2}\nonumber \\&\quad +9\,{{ \rho _d}}^{2} +24\,{ \rho _d}\,\rho _r+16\,{\rho _r}^{2}\bigg ]\;, \end{aligned}$$
(97)
$$\begin{aligned}&f_3 \left( T \right) = \frac{1}{9\, {{ \rho _d}}^{2}+24\,{ \rho _d}\,\rho _r+16\,{\rho _r}^{2}+36\,A}\bigg \{ 9\,{{ \rho _d}}^{2}T\nonumber \\&\quad +24\,{ \rho _d}\, \rho _r\,T +16\,{\rho _r}^{2}T+36\,A{ \rho _d}+24\,A\rho _r \nonumber \\&\quad -2\,\bigg [162\,A{{ \rho _d}}^ {3}T+108\,A{{ \rho _d}}^{3}\rho _r-81\,A{{ \rho _d}}^{2}{T}^{2}\nonumber \\&\quad +540\, A{{ \rho _d}}^{2}T\rho _r+396\,A{{ \rho _d}}^{2}{\rho _r}^{2}-216\,A{ \rho _d}\,{T }^{2}\rho _r \nonumber \\&\quad +576\,A{ \rho _d}\,T{\rho _r}^{2}+480\,A{ \rho _d}\,{\rho _r}^{3}-144 \,A{T}^{2}{\rho _r}^{2}\nonumber \\&\quad +192\,AT{\rho _r}^{3}+192\,A{\rho _r}^{4}+324\,{A} ^{2}{{ \rho _d}}^{2}\nonumber \\&\quad +864\,{A}^{2}{ \rho _d}\,\rho _r +576\,{A}^{2}{\rho _r}^{2} \bigg ]^{\frac{1}{2}}\bigg \}\;, \end{aligned}$$
(98)
$$\begin{aligned}&f_4 \left( T \right) = \frac{1}{9\, {{ \rho _d}}^{2}+24\,{ \rho _d}\,\rho _r+16\,{\rho _r}^{2}+36\,A}\bigg \{ 9\,{{ \rho _d}}^{2}T\nonumber \\&\quad +24\,{ \rho _d}\, \rho _r\,T +16\,{\rho _r}^{2}T+36\,A{ \rho _d}+24\,A\rho _r \nonumber \\&\quad +2\,\bigg [162\,A{{ \rho _d}}^ {3}T+108\,A{{ \rho _d}}^{3}\rho _r-81\,A{{ \rho _d}}^{2}{T}^{2}\nonumber \\&\quad +540\, A{{ \rho _d}}^{2}T\rho _r+396\,A{{ \rho _d}}^{2}{\rho _r}^{2}-216\,A{ \rho _d}\,{T }^{2}\rho _r\nonumber \\&\quad +576\,A{ \rho _d}\,T{\rho _r}^{2}+480\,A{ \rho _d}\,{\rho _r}^{3}-144 \,A{T}^{2}{\rho _r}^{2}\nonumber \\&\quad +192\,AT{\rho _r}^{3}+192\,A{\rho _r}^{4}+324\,{A} ^{2}{{ \rho _d}}^{2}\nonumber \\&\quad +864\,{A}^{2}{ \rho _d}\,\rho _r +576\,{A}^{2}{\rho _r}^{2} \bigg ]^{\frac{1}{2}}\bigg \}. \end{aligned}$$
(99)
If \(\rho _d = \rho _r = 0\), the above to f(T) gravity models Eqs. (96) and (97) reduce to the vacuum case Eq. (23) and (24) respectively. The other two solutions Eqs. (98) and (99) go to zero in the vacuum limiting case. We substitute \(f_1(T)\), \(f_2(T)\), \(f_3(T)\) and \(f_4(T)\) into Eq. (7). Then, the energy density of the torsion fluid in radiation-dust-torsion system:
$$\begin{aligned}& \rho _T^1 = \,{\frac{-\varpi + \left( -3\, { \rho _d}-4\,\rho _r \right) { c}+3\,{ \rho _d}+4\,\rho _r}{6{ c}} }\;, \end{aligned}$$
(100)
$$\begin{aligned}& \rho _T^2 = \,{\frac{\varpi + \left( -3\, { \rho _d}-4\,\rho _r \right) { c}+3\,{ \rho _d}+4\,\rho _r}{6{ c}} }\;, \end{aligned}$$
(101)
$$\begin{aligned}& \rho _T^3 = 2\,{\frac{A \left( 6\, \left( { \rho _d}+4/3\,\rho _r \right) \left( 2/3 \,{\rho _r}^{2}+ \left( -T/3+7/6\,{ \rho _d} \right) \rho _r-1/4\,{ \rho _d}\, T+1/2\,{{ \rho _d}}^{2}+A \right) \sqrt{3}+ \mathscr {N}\right) }{ \left( { \rho _d}+4/3\,\rho _r \right) \left( 6\,A \left( T-{ \rho _d}-2/3\,\rho _r \right) \sqrt{3}+ \mathscr {N}\right) }}\;, \end{aligned}$$
(102)
$$\begin{aligned}& \rho _T^4 = 2\,{\frac{A \left( -6\, \left( { \rho _d}+4/3\,\rho _r \right) \left( 2/ 3\,{\rho _r}^{2}+ \left( -T/3+7/6\,{ \rho _d} \right) \rho _r-1/4\,{ \rho _d} \,T+1/2\,{{ \rho _d}}^{2}+A \right) \sqrt{3}+\mathscr {N} \right) }{ \left( { \rho _d}+4/3\,\rho _r \right) \left( -6\,A \left( T-{ \rho _d} -2/3\,\rho _r \right) \sqrt{3}+\mathscr {N} \right) }}, \end{aligned}$$
(103)
where
$$\begin{aligned} \varpi= & {} \sqrt{9\, \left( { c}-1 \right) ^{2}{{ \rho _d}}^{ 2}+24\,\rho _r\, \left( { c}-1 \right) ^{2}{ \rho _d}+16\, \left( { c}-1 \right) ^{2}{\rho _r}^{2}+36\,A{{ c}}^{2}} \\ \mathscr {N}= & {} \sqrt{ \left( 3\,{ \rho _d}+4\,\rho _r \right) ^{2}A \left( 6\,{ \rho _d}\,T+4\,{ \rho _d}\, \rho _r-3\,{T}^{2}+4\,\rho _r\,T+4\,{\rho _r}^{2}+12\,A \right) }. \end{aligned}$$
And we also substitute \(f_1(T)\), \(f_2(T)\), \(f_3(T)\) and \(f_4(T)\) into Eq. (9), and reconstruct the correspond pressure of the fluid given as follows:
$$\begin{aligned}&\rho _T = \,{\frac{\varpi + \left( -9\, { \rho _d}-8\,\rho _r \right) { c}+9\,{ \rho _d}+8\,\rho _r}{6{ c}} }\;, \end{aligned}$$
(104)
$$\begin{aligned}&\rho _T = - \,{\frac{\varpi + \left( -9\, { \rho _d}-8\,\rho _r \right) { c}+9\,{ \rho _d}+8\,\rho _r}{6{ c}} }\;, \end{aligned}$$
(105)
$$\begin{aligned}&p_T^3 = \,{\frac{A -\left( 2\, \left( { \rho _d}+\frac{4}{3}\,\rho _r \right) ^{2} \left( \left( \frac{2}{3}\,T-{ \rho _d}/2 \right) \rho _r+\frac{3}{4}\,{ \rho _d}\, T-1/2 \,{{ \rho _d}}^{2}+A \right) \sqrt{3}+1/9 \mathscr {N} \left( 9\,{ \rho _d}+8\, \rho _r \right) \right) }{ 6\left( { \rho _d}+4/3\,\rho _r \right) ^{2} \left( -6\,A \left( T-{ \rho _d}-\frac{2}{3}\,\rho _r \right) \sqrt{3}+ \mathscr {N} \right) }}\;, \end{aligned}$$
(106)
$$\begin{aligned}&p_T^4 = \,{\frac{A \left( 2\, \left( { \rho _d}+\frac{4}{3}\,\rho _r \right) ^{2} \left( \left( \frac{2}{3}\,T-{ \rho _d}/2 \right) \rho _r+\frac{3}{4}\,{ \rho _d}\, T-1/2 \,{{ \rho _d}}^{2}+A \right) \sqrt{3}+1/9 \mathscr {N} \left( 9\,{ \rho _d}+8\, \rho _r \right) \right) }{ 6\left( { \rho _d}+4/3\,\rho _r \right) ^{2} \left( -6\,A \left( T-{ \rho _d}-\frac{2}{3}\,\rho _r \right) \sqrt{3}+ \mathscr {N} \right) }}. \end{aligned}$$
(107)
And the corresponding equation of state parameter of the torsion fluid express as follows:
$$\begin{aligned}&w^1_T = {\frac{ \left( 9\,{ \rho _d}+8\,\rho _r \right) { c}+\varpi -9\,{ \rho _d}-8\,\rho _r}{ \left( 3\,{ \rho _d}+4\,\rho _r \right) { c}-\varpi -3\,{ \rho _d}-4\,\rho _r}},\\&w^2_T = {\frac{ \left( 9\,{ \rho _d}+8\,\rho _r \right) { c}-\varpi -9\,{ \rho _d}-8\,\rho _r}{ \left( 3\,{ \rho _d}+4\,\rho _r \right) { c}+\varpi -3\,{ \rho _d}-4\,\rho _r}}, \\&w^3_T = \,{\frac{-108\, \left( { \rho _d}+4/3\,\rho _r \right) ^{2} \left( \left( 2/3\,T-{ \rho _d}/2 \right) \rho _r+3/4\,{ \rho _d}\,T-1/2\,{ { \rho _d}}^{2}+A \right) \sqrt{3}+6\,\mathscr {N} }{ 18\left( { \rho _d}+4/3\,\rho _r \right) \bigg ( 6\, \left( { \rho _d}+4/3\,\rho _r \right) \left( 2/3\,{\rho _r}^{2}+ \left( - T/3+7/6\,{ \rho _d} \right) \rho _r-1/4\,{ \rho _d}\,T+1/2\,{{ \rho _d}}^{2}+A \right) \sqrt{3}+ \mathscr {N} \bigg ) }} , \\&w^4_T = \,{\frac{108\, \left( { \rho _d}+4/3\,\rho _r \right) ^{2} \left( \left( 2/3\,T-{ \rho _d}/2 \right) \rho _r+3/4\,{ \rho _d}\,T-1/2\,{ { \rho _d}}^{2}+A \right) \sqrt{3}+6\,\mathscr {N} }{ 18\left( { \rho _d}+4/3\,\rho _r \right) \bigg ( 6\, \left( { \rho _d}+4/3\,\rho _r \right) \left( 2/3\,{\rho _r}^{2}+ \left( - T/3+7/6\,{ \rho _d} \right) \rho _r-1/4\,{ \rho _d}\,T+1/2\,{{ \rho _d}}^{2}+A \right) \sqrt{3}+ \mathscr {N} \bigg ) }}. \end{aligned}$$
We present the numerical plots of the evolution of effective equation of state parameter in Fig. 5 for non-interacting fluids (radiation-dust-torsion systems). Here we reconstruct the fraction of energy densities for torsion fluid in radiation-dust-torsion system as follows:
$$\begin{aligned}&\xi _1 = \frac{ \, {-\varpi + \left( -3\, { \rho _d}-4\,\rho _r \right) { c}+3\,{ \rho _d}+4\,\rho _r}{}}{ \, {-\varpi + \left( -3\, { \rho _{d,0}}-4\,\rho _{r,0} \right) { c}+3\,{ \rho _{d,0}}+4\,\rho _{r,0}}{}} \;,\nonumber \\ \end{aligned}$$
(108)
$$\begin{aligned}&\xi _2 = \,{\frac{\sqrt{9\, \left( { c}-1 \right) ^{2}{{ \rho _d}}^{ 2}+24\,\rho _r\, \left( { c}-1 \right) ^{2}{ \rho _d}+16\, \left( { c}-1 \right) ^{2}{\rho _r}^{2}+36\,A{{ c}}^{2}}+ \left( -3\, { \rho _d}-4\,\rho _r \right) { c}+3\,{ \rho _d}+4\,\rho _r}{\sqrt{9\, \left( { c}-1 \right) ^{2}{{ \rho _{d,0}}}^{ 2}+24\,\rho _{r,0}\, \left( { c}-1 \right) ^{2}{ \rho _{d,0}}+16\, \left( { c}-1 \right) ^{2}{\rho _{r,0}}^{2}+36\,A{{ c}}^{2}}+ \left( -3\, { \rho _{d,0}}-4\,\rho _{r,0} \right) { c}+3\,{ \rho _{d,0}}+4\,\rho _{r,0}} } \;,\nonumber \\ \end{aligned}$$
(109)
$$\begin{aligned}&\xi _3 = \frac{2\,{\frac{A \left( 6\, \left( { \rho _d}+4/3\,\rho _r \right) \left( 2/3 \,{\rho _r}^{2}+ \left( -T/3+7/6\,{ \rho _d} \right) \rho _r-1/4\,{ \rho _d}\, T+1/2\,{{ \rho _d}}^{2}+A \right) \sqrt{3}+ \mathscr {N}\right) }{ \left( { \rho _d}+4/3\,\rho _r \right) \left( 6\,A \left( T-{ \rho _d}-2/3\,\rho _r \right) \sqrt{3}+ \mathscr {N}\right) }}}{ 2\,{\frac{A \left( 6\, \left( { \rho _{d,0}}+4/3\,\rho _{r,0} \right) \left( 2/3 \,{\rho _{r,0}}^{2}+ \left( -T/3+7/6\,{ \rho _{d,0}} \right) \rho _{r,0}-1/4\,{ \rho _{d,0}}\, T+1/2\,{{ \rho _{d,0}}}^{2}+A \right) \sqrt{3}+ \mathscr {N}\right) }{ \left( { \rho _{d,0}}+4/3\,\rho _{r,0} \right) \left( 6\,A \left( T-{ \rho _{d,0}}-2/3\,\rho _{r,0} \right) \sqrt{3}+ \mathscr {N}\right) }}} \;, \end{aligned}$$
(110)
$$\begin{aligned}&\xi _4 = \frac{2\,{\frac{A \left( -6\, \left( { \rho _d}+4/3\,\rho _r \right) \left( 2/3 \,{\rho _r}^{2}+ \left( -T/3+7/6\,{ \rho _d} \right) \rho _r-1/4\,{ \rho _d}\, T+1/2\,{{ \rho _d}}^{2}+A \right) \sqrt{3}+ \mathscr {N}\right) }{ \left( { \rho _d}+4/3\,\rho _r \right) \left( - 6\,A \left( T-{ \rho _d}-2/3\,\rho _r \right) \sqrt{3}+ \mathscr {N}\right) }}}{ 2\,{\frac{A \left( - 6\, \left( { \rho _{d,0}}+4/3\,\rho _{r,0} \right) \left( 2/3 \,{\rho _{r,0}}^{2}+ \left( -T/3+7/6\,{ \rho _{d,0}} \right) \rho _{r,0}-1/4\,{ \rho _{d,0}}\, T+1/2\,{{ \rho _{d,0}}}^{2}+A \right) \sqrt{3}+ \mathscr {N}\right) }{ \left( { \rho _{d,0}}+4/3\,\rho _{r,0} \right) \left( - 6\,A \left( T-{ \rho _{d,0}}-2/3\,\rho _{r,0} \right) \sqrt{3}+ \mathscr {N}\right) }}}\;, \end{aligned}$$
(111)
$$\begin{aligned}&\chi _1 = \frac{\mathscr {J}\, {-\varpi + \left( -3\, { \rho _d}-4\,\rho _r \right) { c}+3\,{ \rho _d}+4\,\rho _r}{}}{ \, { \mathscr {J} -\varpi + \left( -3\, { \rho _{d,0}}-4\,\rho _{r,0} \right) { c}+3\,{ \rho _{d,0}}+4\,\rho _{r,0}}{}}\;, \end{aligned}$$
(112)
$$\begin{aligned}&\chi _2 = \,{\frac{\mathscr {J} + \varpi + \left( -3\, { \rho _d}-4\,\rho _r \right) { c}+3\,{ \rho _d}+4\,\rho _r}{ \mathscr {J}+ \varpi + \left( -3\, { \rho _{d,0}}-4\,\rho _{r,0} \right) { c}+3\,{ \rho _{d,0}}+4\,\rho _{r,0}} } \;, \end{aligned}$$
(113)
$$\begin{aligned}&\chi _3 = \frac{ \rho _d + \rho _r +2\,{\frac{A \left( 6\, \left( { \rho _d}+4/3\,\rho _r \right) \left( 2/3 \,{\rho _r}^{2}+ \left( -T/3+7/6\,{ \rho _d} \right) \rho _r-1/4\,{ \rho _d}\, T+1/2\,{{ \rho _d}}^{2}+A \right) \sqrt{3}+ \mathscr {N}\right) }{ \left( { \rho _d}+4/3\,\rho _r \right) \left( 6\,A \left( T-{ \rho _d}-2/3\,\rho _r \right) \sqrt{3}+ \mathscr {N}\right) }}}{\rho _{d,0} + \rho _{r,0} + 2\,{\frac{A \left( 6\, \left( { \rho _{d,0}}+4/3\,\rho _{r,0} \right) \left( 2/3 \,{\rho _{r,0}}^{2}+ \left( -T/3+7/6\,{ \rho _{d,0}} \right) \rho _{r,0}-1/4\,{ \rho _{d,0}}\, T+1/2\,{{ \rho _{d,0}}}^{2}+A \right) \sqrt{3}+ \mathscr {N}\right) }{ \left( { \rho _{d,0}}+4/3\,\rho _{r,0} \right) \left( 6\,A \left( T-{ \rho _{d,0}}-2/3\,\rho _{r,0} \right) \sqrt{3}+ \mathscr {N}\right) }}} \;, \end{aligned}$$
(114)
$$\begin{aligned}&\chi _4 = \frac{ \rho _d + \rho _r +2\,{\frac{A \left( -6\, \left( { \rho _d}+4/3\,\rho _r \right) \left( 2/3 \,{\rho _r}^{2}+ \left( -T/3+7/6\,{ \rho _d} \right) \rho _r-1/4\,{ \rho _d}\, T+1/2\,{{ \rho _d}}^{2}+A \right) \sqrt{3}+ \mathscr {N}\right) }{ \left( { \rho _d}+4/3\,\rho _r \right) \left( - 6\,A \left( T-{ \rho _d}-2/3\,\rho _r \right) \sqrt{3}+ \mathscr {N}\right) }}}{ \rho _{d,0} + \rho _{r,0} 2\,{\frac{A \left( - 6\, \left( { \rho _{d,0}}+4/3\,\rho _{r,0} \right) \left( 2/3 \,{\rho _{r,0}}^{2}+ \left( -T/3+7/6\,{ \rho _{d,0}} \right) \rho _{r,0}-1/4\,{ \rho _{d,0}}\, T+1/2\,{{ \rho _{d,0}}}^{2}+A \right) \sqrt{3}+ \mathscr {N}\right) }{ \left( { \rho _{d,0}}+4/3\,\rho _{r,0} \right) \left( - 6\,A \left( T-{ \rho _{d,0}}-2/3\,\rho _{r,0} \right) \sqrt{3}+ \mathscr {N}\right) }}} \;, \end{aligned}$$
(115)
where
$$\begin{aligned} \mathscr {J} = 6c \rho _d + 6c \rho _r. \end{aligned}$$
We present the behavior of the fractional energy densities in Fig. 6.
2.2 Reconstructing modified teleparallel gravity from the GCG model
The frame-work of the GCG in the modified theory of gravity was first proposed by Rastall [40]. Here, we consider the general model of CG model to reconstruct f(T) gravity model and the corresponding thermodynamical quantities of the torsion fluid. Similar to our previous discussions for the OCG model, we consider five cases, namely vacuum, radiation-torsion, dust-torsion, stiff matter-torsion and radiation-dust-torsion systems.
2.2.1 Vacuum case
Here we assume that the vacuum Universe and the energy density and pressure of the matter fluid are negligible, i,e., \(p_m = \rho _m = 0\). The general expression of Eq. (17) in vacuum system is given as
$$\begin{aligned}&\left[ -\frac{1}{f'}\right] ^{1+\alpha }\left[ -\frac{1}{2}(f-Tf')\right] ^{1+\alpha }=-A, \end{aligned}$$
(116)
and we can reconstruct the f(T) gravity model from this expression and it is given by
$$\begin{aligned}&f(T ) = c \left[ T- 2(-A)^{\frac{1}{1+\alpha }}\right] . \end{aligned}$$
(117)
In most cases, we have \(\alpha \) as a positive constant, with a value between 0 to 1. However, in the literature [41,42,43,44,45,46], the value of \(\alpha \) can be a free parameter and larger than \(-1\). If, in our case, \(\alpha ={1}/{2}\), the reconstructed f(T) gravity model in Eq. (117) becomes imaginary, \(f(T ) = cT- 2ic\sqrt{A}\); on the other hand, if \(\alpha =-{1}/{2}\), then \(f(T ) = cT- 2c\sqrt{A}\) and this solution is exactly the same as the selected solution in the OCG model, Eq. (23). This is our motivation to account for the parameter \(\alpha \) as being either positive or negative. Based on the claim of [41, 43,44,45,46] and the above motivation, \(\alpha \) can be a negative number \(\alpha \ge -1\). Then, we choose the parameter \(\alpha =-1/2\), the reconstructed f(T) function in GCG in Eq. (117) is reduced to OCG in Eq. (23). Based on this suggestion, we have set the value of \(\alpha = -1/2\) in this paper for further investigation of different f(T) gravity models, to manifest the cosmological implication of the corresponding thermodynamical quantities. Therefore, this f(T) which is presented in Eq. (117) is the general of the Eq. (23). By substituting Eq. (117) into Eqs. (7) and (9), it could be reconstruct the energy density, pressure and the corresponding equation of state for torsion fluid in the vacuum system.
2.2.2 Radiation-torsion system
Here we consider the radiation-torsion system in GCG model, and radiation with torsion component is considered as an exotic fluid to lead the cosmic expansion. The energy density and pressure of the fluid has been involving from the early to late Universe as a constant and which are presented in Eqs. (7) and (9). The general expression of Eq. (17) for radiation-torsion system is given by
$$\begin{aligned}&-\frac{1}{f'}\left[ (f'-1)\frac{\rho _r}{3} -\frac{1}{2}(f-Tf')\right] \nonumber \\&\quad \bigg [-\frac{1}{f'}\left( (f'-1)\rho _r +\frac{1}{2}(f-Tf')\right) \bigg ]^\alpha =-A. \end{aligned}$$
(118)
Then, by applying the same reasoning as vacuum case, we set the value of \(\alpha = -1/2\), to reconstruct different f(T) gravity models in the below:
$$\begin{aligned}&f_{1} \left( T \right) =cT+\frac{1}{3}\left( 2c\rho _r+Ac^{2} \left( 3\,A\right. \right. \nonumber \\&\quad -\left. \left. \sqrt{3}\sqrt{{\frac{3\,{A}^{ 2}{ c}-16\,\rho _r\,{ c}+16\,\rho _r}{{ c}}}} \right) -2\rho _r \right) \;, \end{aligned}$$
(119)
$$\begin{aligned}&f_{2} \left( T \right) =cT+\frac{1}{3}\left( 2c\rho _r+Ac^{2} \left( 3\,A\right. \right. \nonumber \\&\quad +\left. \left. \sqrt{3}\sqrt{{\frac{3\,{A}^{ 2}{ c}-16\,\rho _r\,{ c}+16\,\rho _r}{{ c}}}} \right) -2\rho _r \right) . \end{aligned}$$
(120)
By substituting \(f_1(T)\) and \(f_2(T)\) into Eq. (7), we obtain the energy density of the torsion fluid \(\rho _{T}^{1}\) and \(\rho _{T}^{2}\). These the energy density of the torsion fluid express as follows:
$$\begin{aligned}&\rho _{T}^{1} = \,\frac{1}{6{ c}} \left( -A\sqrt{3}\sqrt{{\frac{ \left( 3 \,{A}^{2}-16\,\rho _r \right) { c}+16\,\rho _r}{{ c}}}}\right. \nonumber \\&\quad +\left. \left( 3\,{A}^{2}-8\,\rho _r \right) { c}+8\,\rho _r \right) , \end{aligned}$$
(121)
$$\begin{aligned}&\rho _{T}^{2} = \,\frac{1}{6{ c}} \left( A\sqrt{3}\sqrt{{\frac{ \left( 3 \,{A}^{2}-16\,\rho _r \right) { c}+16\,\rho _r}{{ c}}}}\right. \nonumber \\&\quad +\left. \left( 3\,{A}^{2}-8\,\rho _r \right) { c}+8\,\rho _r \right) . \end{aligned}$$
(122)
In the limiting case of \(\rho _r =0\), the function \(f_1(T)\) in Eq. (119) and the energy density of the torsion fluid \(\rho ^{T}_{1}\) in Eq. (121) are reduced to vacuum case while, the function \(f_2(T)\) in Eq. (120) and the energy density of the torsion fluid \(\rho ^{T}_{2}\) in Eq. (122) go to zero. Here, we also reconstruct the corresponding pressure of the torsion fluid during radiation-torsion system by substituting \(f_1(T)\) and \(f_2(T)\) into Eq. (9) and we have
$$\begin{aligned}&p_{T}^{1} =\,\frac{1}{6{ c}} \left( A\sqrt{3}\sqrt{{\frac{ \left( 3 \,{A}^{2}-16\,\rho _r \right) { c}+16\,\rho _r}{{ c}}}}\right. \nonumber \\&\quad + \left. \left( -3\,{A}^{2}-4\,\rho _r \right) { c}+4\,\rho _r \right) , \end{aligned}$$
(123)
$$\begin{aligned}&p_{T}^{2} =\,\frac{1}{6{ c}} \left( -A\sqrt{3}\sqrt{{\frac{ \left( 3 \,{A}^{2}-16\,\rho _r \right) { c}+16\,\rho _r}{{ c}}}}\right. \nonumber \\&\quad +\left. \left( -3\,{A}^{2}-4\,\rho _r \right) { c}+4\,\rho _r \right) , \end{aligned}$$
(124)
and the equation of state parameter \(w_T\) of the torsion fluid is given as
$$\begin{aligned}&w_{T}^{1} = \frac{ A\sqrt{3}\sqrt{{\frac{ \left( 3\,{A}^{2}-16\,\rho _r \right) { c}+16\,\rho _r}{{ c}}}}{}+ \left( -3\,{A}^ {2}-4\,\rho _r \right) { c}+4\,\rho _r }{-A\sqrt{3} \sqrt{{\frac{ \left( 3\,{A}^{2}-16\,\rho _r \right) { c}+16\,\rho _r }{{ c}}}}{}+ \left( 3\,{A}^{2}-8\,\rho _r \right) { c }+8\,\rho _r },\nonumber \\ \end{aligned}$$
(125)
$$\begin{aligned}&w_{T}^{2} = \frac{-A\sqrt{3}\sqrt{{\frac{ \left( 3\,{A}^{2}-16\,\rho _r \right) { c}+16\,\rho _r}{{ c}}}}{ c}+ \left( -3\,{A}^ {2}-4\,\rho _r \right) { c}+4\,\rho _r }{ A\sqrt{3} \sqrt{{\frac{ \left( 3\,{A}^{2}-16\,\rho _r \right) { c}+16\,\rho _r }{{ c}}}}{}+ \left( 3\,{A}^{2}-8\,\rho _r \right) { c }+8\,\rho _r }.\nonumber \\ \end{aligned}$$
(126)
We use the definition of Eq. (18) and the numerical plots of the equation of state parameter for the radiation-torsion system is presented in Fig. 7 for GCG.
In the similar mathematical manipulation as OCG in GCG we also obtain the growth factor parameters by taking the ratio of the energy density of torsion fluid \(\xi \) and effective fluid \(\chi \). These the growth factor parameters are given as follows:
$$\begin{aligned} \xi _{1}= & {} \frac{ -A\sqrt{3}\sqrt{{\frac{ \left( 3\,{A}^{2}-16\,\rho _r \right) { c}+16\,\rho _r}{{ c}}}}{ c}+ \left( 3\,{A}^{ 2}-8\,\rho _r \right) { c}+8\,\rho _r}{ -A\sqrt{3} \sqrt{{\frac{ \left( 3\,{A}^{2}-16\,\rho _{r,0} \right) { c}+16\, \rho _{r,0}}{{ c}}}}{ c}+ \left( 3\,{A}^{2}-8\,\rho _{r,0} \right) { c}+8\,\rho _{r,0} } \;,\nonumber \\ \end{aligned}$$
(127)
$$\begin{aligned} \xi _{2}= & {} \frac{ A\sqrt{3}\sqrt{{\frac{ \left( 3\,{A}^{2}-16\,\rho _r \right) { c}+16\,\rho _r}{{ c}}}}{ c}+ \left( 3\,{A}^{ 2}-8\,\rho _r \right) { c}+8\,\rho _r}{ -A\sqrt{3} \sqrt{{\frac{ \left( 3\,{A}^{2}-16\,\rho _{r,0} \right) { c}+16\, \rho _{r,0}}{{ c}}}}{ c}+ \left( 3\,{A}^{2}-8\,\rho _{r,0} \right) { c}+8\,\rho _{r,0}} \;,\nonumber \\ \end{aligned}$$
(128)
$$\begin{aligned} \chi _{1}= & {} \frac{\rho _r -A\sqrt{3}\sqrt{{\frac{ \left( 3\,{A}^{2}-16\,\rho _r \right) { c}+16\,\rho _r}{{ c}}}}{ c}+ \left( 3\,{A}^{ 2}-2\,\rho _r \right) { c}+8\,\rho _r}{\rho _{r,0} -A\sqrt{3} \sqrt{{\frac{ \left( 3\,{A}^{2}-16\,\rho _{r,0} \right) { c}+16\, \rho _{r,0}}{{ c}}}}{ c}+ \left( 3\,{A}^{2}-2\,\rho _{r,0} \right) { c}+8\,\rho _{r,0} } \;,\nonumber \\ \end{aligned}$$
(129)
$$\begin{aligned} \chi _{2}= & {} \frac{\rho _r+ A\sqrt{3}\sqrt{{\frac{ \left( 3\,{A}^{2}-16\,\rho _r \right) { c}+16\,\rho _r}{{ c}}}}{ c}+ \left( 3\,{A}^{ 2}-2\,\rho _r \right) { c}+8\,\rho _r }{\rho _{r,0} -A\sqrt{3} \sqrt{{\frac{ \left( 3\,{A}^{2}-16\,\rho _{r,0} \right) { c}+16\, \rho _{r,0}}{{ c}}}}{ c}+ \left( 3\,{A}^{2}-2\,\rho _{r,0} \right) { c}+8\,\rho _{r,0} }\;.\nonumber \\ \end{aligned}$$
(130)
The Eqs. (127) and (129) are presented on the left side of Fig. 8, and Eqs. (128) and (130) are presented on the right side of Fig. 8.
2.2.3 Dust-torsion system
In this section, we also consider that dust-torsion system in GCG model and dust and torsion component are considering as an exotic fluids to reconstruct f(T) gravity model. Then, Eq. (17) is given as
$$\begin{aligned}&\left[ f-Tf'\right] \bigg [\left( f'-1\right) \rho _d +\frac{1}{2}\left( f-Tf'\right) \bigg ]^\alpha \nonumber \\&\quad -2(-1)^{(1+\alpha )}\left( f'\right) ^{(1+\alpha )}A=0 \;. \end{aligned}$$
(131)
By setting the \(\alpha = -1/2\), the solutions of Eq. (131) are given as follows:
$$\begin{aligned}&f_1(T) = -{ c}\, \left( {A}^{2}+A\sqrt{{\frac{ \left( {A}^{2}-4\, \rho _d \right) { c}+4\,\rho _d}{{ c}}}}-T \right) \;,\nonumber \\ \end{aligned}$$
(132)
$$\begin{aligned}&f_2(T) = { c}\, \left( A\sqrt{{\frac{ \left( {A}^{2}-4\,\rho _d \right) { c}+4\,\rho _d}{{ c}}}}-{A}^{2}+T \right) \;.\nonumber \\ \end{aligned}$$
(133)
Based on the above reconstructed functions \(f_1(T)\) and \(f_2(T)\), we also reconstruct the energy density of the torsion fluid as follows
$$\begin{aligned}&\rho _{T}^{1} = \,\frac{1}{{ 2c}} \left[ \left( -2\,\rho _d\right. \right. \nonumber \\&\quad +\left. \left. A \left( \sqrt{{ \frac{ \left( {A}^{2}-4\,\rho _d \right) { c}+4\,\rho _d}{{ c}} }}+A \right) \right) { c}+2\,\rho _d \right] \;,\nonumber \\ \end{aligned}$$
(134)
and
$$\begin{aligned}&\rho ^2_T = \,\frac{1}{{ 2c}} \left[ \left( -2\,\rho _d\right. \right. \nonumber \\&\quad -\left. \left. A \left( \sqrt{{ \frac{ \left( {A}^{2}-4\,\rho _d \right) { c}+4\,\rho _d}{{ c}} }}-A \right) \right) { c}+2\,\rho _d \right] \;.\nonumber \\ \end{aligned}$$
(135)
By substituting \(f_1(T)\) and \(f_2(T)\) in Eq. (9) we reconstruct the pressure of the torsion fluid as follows:
$$\begin{aligned}&p^1_T = \,\frac{1}{2{ c}} \left[ \left( -2\,\rho _d\right. \right. \nonumber \\&\quad -\left. \left. A \left( \sqrt{{ \frac{ \left( {A}^{2}-4\,\rho _d \right) { c}+4\,\rho _d}{{ c}} }}+A \right) \right) { c}+2\,\rho _d \right] \;,\nonumber \\ \end{aligned}$$
(136)
$$\begin{aligned}&p_{T}^{2} = \,\frac{1}{2{ c}} \left[ \left( -2\,\rho _d\right. \right. \nonumber \\&\quad +\left. \left. A \left( \sqrt{{ \frac{ \left( {A}^{2}-4\,\rho _d \right) { c}+4\,\rho _d}{{ c}} }}-A \right) \right) { c}+2\,\rho _d \right] \;.\nonumber \\ \end{aligned}$$
(137)
From the reconstructed energy density and pressure of the fluid we have to obtain the following equation of state parameters of torsion fluid in dust dominated case
$$\begin{aligned}&w_T^1 = -\frac{ 2\,\rho _d -A \sqrt{{\frac{ \left( {A}^ {2}-4\, \rho _d \right) { c}+4\,\rho _d}{{ c}}}}-A { c}-2\,\rho _d}{2\,\rho _d-A \sqrt{{ \frac{ \left( {A}^{2}-4\,\rho _d \right) { c}+4\,\rho _d}{{ c}} }}-A { c}-2\,\rho _d } \;,\nonumber \\ \end{aligned}$$
(138)
$$\begin{aligned}&w_{T}^{2}= \frac{ \left[ 2\,\rho _d-A \left( \sqrt{{\frac{ \left( {A}^ {2}-4\, \rho _d \right) { c}+4\,\rho _d}{{ c}}}}-A \right) \right] { c}-2\,\rho _d }{ \left[ 2\,\rho _d+A \left( \sqrt{{ \frac{ \left( {A}^{2}-4\,\rho _d \right) { c}+4\,\rho _d}{{ c}} }}-A \right) \right] { c}-2\,\rho _d } \;.\nonumber \\ \end{aligned}$$
(139)
We use the definition of Eq. (18) and the numerical plots of the equation of state parameter for the dust-torsion system is presented in Fig. 9 for GCG.
By applying the same reason as radiation dominated case, the growth factor parameters of the fluid are given as follows:
$$\begin{aligned}&\xi _{1}=\frac{ -A\sqrt{{\frac{ \left( {A}^{2}-4\,\rho _d \right) { c}+ 4\,\rho _d}{{ c}}}}{ c}+ \left( {A}^{2}-2\,\rho _d \right) { c}+2\,\rho _d }{ \left( A\sqrt{{\frac{ \left( {A}^{2}- 4\,\rho _{d,0} \right) { c}+4\,\rho _{d,0}}{{ c}}}}+{A}^{2}-2\,\rho _{d,0} \right) { c}+2\,\rho _{d,0} }\;,\nonumber \\ \end{aligned}$$
(140)
$$\begin{aligned}&\xi _{2}= \frac{ A{ c}\,\sqrt{{\frac{ \left( {A}^{2}-4\,\rho _d \right) { c}+4\,\rho _d}{{ c}}}}+ \left( {A}^{2}-2\,\rho _d \right) { c}+2\,\rho _d }{ \left( A\sqrt{{\frac{ \left( {A}^ {2}-4\,\rho _{d,0} \right) { c}+4\,\rho _{d,0}}{{ c}}}}+{A}^{2}-2\, \rho _{d,0} \right) { c}+2\,\rho _{d,0}}\;,\nonumber \\ \end{aligned}$$
(141)
$$\begin{aligned}&\chi _{1}= \frac{ {A}^{2}{ c}-A\sqrt{{\frac{ \left( {A}^{2}-4\,\rho _d \right) { c}+4\,\rho _d}{{ c}}}}{ c}+2\,\rho _d }{ A{ c}\, \left( \sqrt{{\frac{ \left( {A}^{2}-4\,\rho _{d,0} \right) { c}+4\,\rho _{d,0}}{{ c}}}}+A \right) +2\,\rho _{d,0}}\;,\nonumber \\ \end{aligned}$$
(142)
$$\begin{aligned}&\chi _{2}= \frac{ {A}^{2}{ c}+A{ c}\,\sqrt{{\frac{ \left( {A}^{2 }-4\,\rho _d \right) { c}+4\,\rho _d}{{ c}}}}+2\,\rho _d}{ A{ c}\, \left( \sqrt{{\frac{ \left( {A}^{2}-4\,\rho _{d,0} \right) { c}+4\,\rho _{d,0}}{{ c}}}}+A \right) +2\,\rho _{d,0}}\;.\nonumber \\ \end{aligned}$$
(143)
If \(\rho _d=0\), all thermodynamical quantities are reduced to the vacuum case. The Eqs. (140) and (142) are presented on the left side of Fig. 10, and Eqs. (141) and (143) are presented on the right side of Fig. 8.
2.2.4 Stiff matter-torsion system
Here, we consider the stiff matter component is considered behind the exotic fluid and the energy density \(\rho _m = \rho _s\) has been involving from the early to late Universe as a constant and which are presented in Eqs. (7)–(9). Then, Eq. (17) is given as which gives
$$\begin{aligned}&-\frac{1}{f'}\left[ (f'-1){\rho _s} -\frac{1}{2}(f-Tf')\right] \nonumber \\&\quad \bigg [-\frac{1}{f'}\left( (f'-1)\rho _s +\frac{1}{2}(f-Tf')\right) \bigg ]^\alpha =-A.\nonumber \\ \end{aligned}$$
(144)
It can be reconstructed different f(T) gravity models by setting \(\alpha = -\frac{1}{2}\) and we have
$$\begin{aligned} f_1(T)= & {} \left( -\sqrt{{\frac{ \left( {A}^{2}-8\,\rho _s \right) { c}+8\, \rho _s}{{ c}}}}A\right. \nonumber \\&-\left. {A}^{2}+T+2\,\rho _s \right) { c}-2\, \rho _s , \end{aligned}$$
(145)
$$\begin{aligned}&f \left( T \right) =\left( \sqrt{{\frac{ \left( {A}^{2}-8\,\rho _s \right) { c}+8\, \rho _s}{{ c}}}}A\right. \nonumber \\&\quad -\left. {A}^{2}+T+2\,\rho _s \right) { c}-2\, \rho _s, \end{aligned}$$
(146)
and also by substituting Eqs. (145) and (146) into Eq. (7) we reconstruct the corresponding energy density of torsion. Then we have
$$\begin{aligned}&\rho ^{T}_{1} = \,\frac{1}{{ 2c}} \left( \left( -4\,\rho _s\right. \right. \nonumber \\&\quad +\left. \left. A \left( \sqrt{{ \frac{ \left( {A}^{2}-8\,\rho _s \right) { c}+8\,\rho _s}{{ c}} }}+A \right) \right) { c}+4\,\rho _s \right) \;,\nonumber \\ \end{aligned}$$
(147)
$$\begin{aligned}&\rho ^2_T = \,\frac{1}{{ 2c}} \left( \left( -4\,\rho _s\right. \right. \nonumber \\&\quad -\left. \left. A \left( \sqrt{{ \frac{ \left( {A}^{2}-8\,\rho _s \right) { c}+8\,\rho _s}{{ c}} }}-A \right) \right) { c}+4\,\rho _s \right) .\nonumber \\ \end{aligned}$$
(148)
By substituting Eqs. (145) and (146) into Eq. (9) we can reconstruct the corresponding pressure of torsion. Then we have
$$\begin{aligned}&p^1_T = -\frac{A}{2} \left( A-\sqrt{{\frac{ \left( {A}^{2}-8\,\rho _s \right) { c}+8\,\rho _s}{{ c}}}} \right) \;, \end{aligned}$$
(149)
$$\begin{aligned}&p^2_T = -\frac{\,A}{2} \left( A+\sqrt{{\frac{ \left( {A}^{2}-8\,\rho _s \right) { c }+8\,\rho _s}{{ c}}}} \right) \;, \end{aligned}$$
(150)
and we also obtain the equation of state parameters as follows:
$$\begin{aligned}&w^1_T = -\frac{{cA} \left( A-\sqrt{{\frac{ \left( {A}^{2}-8\,\rho _s \right) { c}+8\,\rho _s}{{ c}}}} \right) }{\left( \left( -4\,\rho _s+A \left( \sqrt{{ \frac{ \left( {A}^{2}-8\,\rho _s \right) { c}+8\,\rho _s}{{ c}} }}+A \right) \right) { c}+4\,\rho _s \right) } \;,\nonumber \\ \end{aligned}$$
(151)
$$\begin{aligned}&w^2_T = \frac{-A{ c} \sqrt{{\frac{ \left( {A}^{2}-8\,\rho _s \right) { c}+8\,\rho _s}{{ c}}}}+A }{ \left( -4\, \rho _s+A \left( \sqrt{{\frac{ \left( {A}^{2}-8\,\rho _s \right) { c}+8\,\rho _s}{{ c}}}}+A \right) \right) { c}+4\,\rho _s}.\nonumber \\ \end{aligned}$$
(152)
2.2.5 Radiation-dust-torsion system
In this section we consider the three non interacting fluid, namely dust, radiation and torsion fluid fluid are the cause behind as an exotic fluid for cosmic expansion. The general expression from Eq. (17)
$$\begin{aligned}&-\frac{1}{f'}\left[ (f'-1)p_m -\frac{1}{2}(f-Tf')\right] \nonumber \\&\quad \bigg [-\frac{1}{f'}\left( (f'-1)\rho _m +\frac{1}{2}(f-Tf')\right) \bigg ]^\alpha =-A\;.\nonumber \\ \end{aligned}$$
(153)
From this equation we reconstruct two basic f(T) gravity models and these models are given by
$$\begin{aligned}&f_{1}(T)=T{ c}+ 2\,{ c}\,p+ A^2\nonumber \\&\quad -\sqrt{{\frac{{A}^{2}{ c}-4\,p{ c}-4\,\rho \,{ c}+4\,p+4\,\rho }{{ c}}}} \big )-2\,p\;, \end{aligned}$$
(154)
$$\begin{aligned}&f_{2}(T)=T{ c}+ 2\,{ c}\,p+ A^2\nonumber \\&\quad +\sqrt{{\frac{{A}^{2}{ c}-4\,p{ c}-4\,\rho \,{ c}+4\,p+4\,\rho }{{ c}}}} \big )-2\,p \;, \end{aligned}$$
(155)
where as, based on these constructed \(f_1(T)\) and \(f_2(T)\) gravity model in Eqs. (154) and (155) we can reconstruct the energy density of the torsion fluid in the non-interacting fluid. By substituting \(f_1(T)\) and \(f_2(T)\) into Eq. (7), we obtain
$$\begin{aligned}&\rho ^{1}_{T}=\frac{1}{{2 c}} \left( \left( -2\,\rho -2\,p\right. \right. \nonumber \\&\quad -\left. \left. A \left( \sqrt{{\frac{ \left( {A}^{2}-4\,p-4\,\rho \right) { c}+4\,p+4 \,\rho }{{ c}}}}-A \right) \right) { c}+2\,p+2\,\rho \right) \;,\nonumber \\ \end{aligned}$$
(156)
$$\begin{aligned} \\&\rho ^{2}_{T}=\frac{1}{{2 c}} \left( \left( -2\,\rho -2\,p\right. \right. \nonumber \\&\quad +\left. \left. A \left( \sqrt{{\frac{ \left( {A}^{2}-4\,p-4\,\rho \right) { c}+4\,p+4 \,\rho }{{ c}}}}+A \right) \right) { c}+2\,p+2\,\rho \right) \;.\nonumber \\ \end{aligned}$$
(157)
Here also we substitute \(f_1(T)\) and \(f_2(T)\) gravity model in Eqs. (154) and (155) into Eq. (9) to reconstruct the pressure of the torsion fluid in radiation-dust case. Then we have
$$\begin{aligned}&p^{1}_{T}=-\frac{A}{2} \left( A-\sqrt{{\frac{ \left( {A}^{2}-4\,p-4\,\rho \right) { c}+4\,p+4\,\rho }{{ c}}}} \right) \;,\nonumber \\ \end{aligned}$$
(158)
$$\begin{aligned}&p^{2}_{T}= -\frac{A}{2} \left( A+ \sqrt{{\frac{ \left( {A}^{2}-4\,p-4\,\rho \right) { c}+4\,p+4\,\rho }{{ c}}}}\right) \;.\nonumber \\ \end{aligned}$$
(159)
The EoS parameters for torsion are given as follows:
$$\begin{aligned} w^{1}_{T}= \frac{-A{ c} \Big ( \sqrt{{\frac{ \left( {A}^{2}-4\,p-4\,\rho \right) { c}+4\,p+4\,\rho }{{ c}}}}-A \Big )}{ \left[ \Big ( 2\,\rho +2\,p+A \Big ( \sqrt{{\frac{ \left( {A}^{2}-4\,p-4\, \rho \right) { c}+4\,p+4\,\rho }{{ c}}}}-A \Big ) \Big ) { c}-2\,p-2\,\rho \right] }\;, \end{aligned}$$
(160)
and
$$\begin{aligned} \begin{aligned} w^{2}_{T}&= \frac{-A{ c} \Big ( \sqrt{{\frac{ \left( {A}^{2}-4\,p-4\,\rho \right) { c}+4\,p+4\,\rho }{{ c}}}}+A \Big )}{ \left[ \Big ( \sqrt{{\frac{ \left( {A}^{2}-4\,p-4\,\rho \right) { c} +4\,p+4\,\rho }{{ c}}}}A+{A}^{2}-2\,p-2\,\rho \Big ) { c}+ 2\,p+2\,\rho \right] }\;. \end{aligned} \end{aligned}$$
(161)
Here, we present the numerical plots of the evolution of effective equation of state parameter in Fig. 11 for radiation-dust-torsion systems.
The effective quantities such as \(\xi _{1,2}\) and \(\chi _{1,2}\) in the following accordingly:
$$\begin{aligned} \xi _{1}= & {} \frac{\Big ( -{ c}\,A\sqrt{3}\sqrt{{\frac{ \left( 3\,{A}^{2}-12 \,{ \rho _{d}}-16\,{ \rho _{r}} \right) { c}+12\,{ \rho _{d}}+16 \,{ \rho _{r}}}{{ c}}}}+ \left( 3\,{A}^{2}-6\,{ \rho _{d}}-8\,{ \rho _{r}} \right) { c} +6\,{ \rho _{d}}+8\,{ \rho _{r}} \Big )}{ \Big ( -{ c}\,A\sqrt{3}\sqrt{{\frac{ \left( 3\,{A}^ {2}-12\,{ \rho _{d,0}}-16\,{ \rho _{r,0}} \right) { c}+12\,{ \rho _{d,0}}+16\,{ \rho _{r,0}}}{{ c}}}}+ \left( 3\,{A}^{2}-6\,{ \rho _{d,0}}-8\,{ \rho _{r,0}} \right) { c}+6\,{ \rho _{d,0}}+8\,{ \rho _{r,0}} \Big )}\;,\qquad \qquad \qquad \qquad \qquad \ \ \, \end{aligned}$$
(162)
$$\begin{aligned} \xi _{2}= & {} \frac{\Big ( { c}\,A\sqrt{3}\sqrt{{\frac{ \left( 3\,{A}^{2}-12\, { \rho _{m}}-16\,{ \rho _{r}} \right) { c}+12\,{ \rho _{m}}+16\, { \rho _{r}}}{{ c}}}}+ \left( 3\,{A}^{2}-6\,{ \rho _{m}}-8\,{ \rho _{r}} \right) { c}+6\,{ \rho _{m}}+8\,{ \rho _{r}} \Big )}{ \Big ( -{ c}\,A\sqrt{3}\sqrt{{\frac{ \left( 3\,{A}^ {2}-12\,{ \rho _{d,0}}-16\,{ \rho _{r,0}} \right) { c}+12\,{ \rho _{d,0}}+16\,{ \rho _{r,0}}}{{ c}}}}+ \left( 3\,{A}^{2}-6\,{ \rho _{d,0}}-8\,{ \rho _{r,0}} \right) { c}+6\,{ \rho _{d,0}}+8\,{ \rho _{r,0}} \Big )}\;, \end{aligned}$$
(163)
$$\begin{aligned} \chi _{1}= & {} \frac{\Big ( \rho _d+\rho _r -{ c}\,A\sqrt{3}\sqrt{{\frac{ \left( 3\,{A}^{2}-12 \,{ \rho _{d}}-16\,{ \rho _{r}} \right) { c}+12\,{ \rho _{d}}+16 \,{ \rho _{r}}}{{ c}}}}+ \left( 3\,{A}^{2}-6\,{ \rho _{d}}-8\,{ \rho _{r}} \right) { c} +6\,{ \rho _{d}}+8\,{ \rho _{r}} \Big )}{ \rho _{d,0}+\rho _{r,0} \Big ( -{ c}\,A\sqrt{3}\sqrt{{\frac{ \left( 3\,{A}^ {2}-12\,{ \rho _{d,0}}-16\,{ \rho _{r,0}} \right) { c}+12\,{ \rho _{d,0}}+16\,{ \rho _{r,0}}}{{ c}}}}+ \left( 3\,{A}^{2}-6\,{ \rho _{d,0}}-8\,{ \rho _{r,0}} \right) { c}+6\,{ \rho _{d,0}}+8\,{ \rho _{r,0}} \Big )}\;, \end{aligned}$$
(164)
$$\begin{aligned} \chi _{2}= & {} \frac{\Big (\rho _d+\rho _r { c}\,A\sqrt{3}\sqrt{{\frac{ \left( 3\,{A}^{2}-12\, { \rho _{m}}-16\,{ \rho _{r}} \right) { c}+12\,{ \rho _{m}}+16\, { \rho _{r}}}{{ c}}}}+ \left( 3\,{A}^{2}-6\,{ \rho _{m}}-8\,{ \rho _{r}} \right) { c}+6\,{ \rho _{m}}+8\,{ \rho _{r}} \Big )}{ \rho _{d,0}+\rho _{r,0} \Big ( -{ c}\,A\sqrt{3}\sqrt{{\frac{ \left( 3\,{A}^ {2}-12\,{ \rho _{d,0}}-16\,{ \rho _{r,0}} \right) { c}+12\,{ \rho _{d,0}}+16\,{ \rho _{r,0}}}{{ c}}}}+ \left( 3\,{A}^{2}-6\,{ \rho _{d,0}}-8\,{ \rho _{r,0}} \right) { c}+6\,{ \rho _{d,0}}+8\,{ \rho _{r,0}} \Big )}. \end{aligned}$$
(165)
Equations (162) and (164) are presented on the left side of Fig. 12, and Eqs. (163) and (165) are presented on the right side of Fig. 12.
2.3 Reconstructing modified teleparallel gravity from the MGCG model
In this section, we consider the generalization of the GCG [27, 47,48,49,50] in the form:
$$ \begin{aligned} p=\beta \rho -(1+\beta )\frac{A}{\rho ^\alpha }, ~~~~~~~ \beta \ne -1 ~ \& ~0. \end{aligned}$$
(166)
In analogy with previous sections, the pressure of the torsion fluid in MGCG is given by
$$\begin{aligned} p_T=\beta \rho _T-(1+\beta )\frac{A}{\rho _T^\alpha }. \end{aligned}$$
(167)
We substitute \(p_T\) and \(\rho _T\) from Eqs. (9) and (7) into Eq. (167), obtaining
$$\begin{aligned}&\frac{1}{(-f')^{(1+\alpha )}}\left[ (f'-1)p_m -\frac{1}{2}(f-Tf')\right] \nonumber \\&\qquad \left[ (f'-1)\rho _m +\frac{1}{2}(f-Tf')\right] ^\alpha \nonumber \\&\quad =\beta \left[ -\frac{1}{f'}\left( (f'-1)\rho _m +\frac{1}{2}(f-Tf')\right) \right] ^{1+\alpha }\nonumber \\&\qquad -(1+\beta )A. \end{aligned}$$
(168)
Then, this equation is the general expression of Eq. (17); it reduces to Eq. (17) by eliminating the parameter \(\beta \). We now reconstruct different f(T) gravity models in the following cases.
2.3.1 Vacuum case
In vacuum case, the energy density and pressure of the matter fluid are neglected, \(p_m = \rho _m=0\), and Eq. (168) yields:
$$\begin{aligned}&\frac{1}{(-f')^{(1+\alpha )}}\left[ -\frac{1}{2}(f-Tf')\right] \left[ \frac{1}{2}(f-Tf')\right] ^\alpha \nonumber \\&\quad =\beta \left[ -\frac{1}{f'}\left( \frac{1}{2}(f-Tf')\right) \right] ^{1+\alpha }-(1+\beta )A\;, \end{aligned}$$
(169)
the solutions of which are
$$\begin{aligned}&f_1\left( T \right) =-2\,{A}^{2}{ c}+T{ c} \nonumber \\&\end{aligned}$$
(170)
For \(\beta =0\), the above function \(f_2(T)\) is equal \(f_1(T)\) and it also coincide with the selected solution of vacuum case in Eq. (23). In order to obtain the energy density of the torsion fluid for this model we substitute Eqs. (170) and (170) into Eq. (7) and it is given by
$$\begin{aligned}&\rho ^1_T = A^2, \qquad \rho ^2_T = {\frac{{A}^{2} \left( \beta +1 \right) ^{2}}{ \left( \beta -1 \right) ^{2}}}, \end{aligned}$$
(171)
and the corresponding pressures can be found by substitute Eqs. (170) and (170) into Eq. (9) as:
$$\begin{aligned}&p^1_T =-A^2, \qquad p^2_T = -{\frac{{A}^{2} \left( \beta +1 \right) ^{2}}{ \left( \beta -1 \right) ^{2}}}. \end{aligned}$$
(172)
It can be shown that the EoS parameter of the fluid asymptotically approaches that of DE.
2.3.2 Radiation-torsion system
In radiation-torsion system in MGCG model, the general expression of the Eq. (168) is
$$\begin{aligned}&\frac{1}{(-f')^{(1+\alpha )}}\left[ (f'-1)\frac{\rho _r}{3} -\frac{1}{2}(f-Tf')\right] \nonumber \\&\qquad \left[ (f'-1)\rho _r +\frac{1}{2}(f-Tf')\right] ^\alpha \nonumber \\&\quad =\beta \left[ -\frac{1}{f'}\left( (f'-1)\rho _r +\frac{1}{2}(f-Tf')\right) \right] ^{1+\alpha }\nonumber \\&\qquad -(1+\beta )A\;. \end{aligned}$$
(173)
By applying the same reasoning as in Sect. 2.2, we set the value of \(\alpha = -1/2\) to reconstruct the f(T) gravity models. Then, we obtain
$$\begin{aligned}& f_{1}(T) ={ c}\,T-\frac{1}{3(1+\beta )}\Big (3\,{A}^{2}{ c}\, \beta +3\,{A}^{2}{ c}+6\,{ c}\,\beta \,\rho _r -2\,\rho _r\,{ c}-6\,\beta \,\rho _r+2\,\rho _r \nonumber \\&\quad -\sqrt{3}\sqrt{ {A}^{2}{ c}\, \left( 1+\beta \right) \left( 3\,{A}^{2}{ c }\,\beta +3\,{A}^{2}{ c}-16\,\rho _r\,{ c}+16\,\rho _r \right) }\Big ), \end{aligned}$$
(174)
$$\begin{aligned}&f_{2}(T) ={ c}\,T-\frac{3\,{A}^{2}{ c}\,{ \beta }^{2}+6\,{A}^{2}{ c}\,\beta +6\,{ c}\,{\beta }^{2}\rho _r+ 3\,{A}^{2}{ c}-4\,{ c}\,\beta \,\rho _r-6\,{\beta }^{2}\rho _r-2\,\rho _r\,{ c}+4\,\beta \,\rho _r+ 2\,\rho _r}{3({\beta }^{2}-2\,\beta +1)}\nonumber \\&\quad +\frac{\sqrt{3}\sqrt{{A}^{2}{ c}\, \left( 1+\beta \right) ^{2} \left( 3\,{A}^{2}{ c}\,{\beta }^{2}+6\,{A}^{2}{ c}\,\beta + 3\,{A}^{2}{ c}+16\,{ c}\,\beta \,\rho _r-16\,\rho _r\,{ c}- 16\,\beta \,\rho _r+16\,\rho _r \right) }}{3({\beta }^{2}-2\,\beta +1)}. \end{aligned}$$
(175)
By substituting \(f_1(T)\) and \(f_2(T)\) gravity models into Eq. (7) we calculate the energy density of the torsion fluid in MGCG as follows:
$$\begin{aligned}& \rho ^{1}_{T}={\frac{-3\,\sqrt{{ c}\, \left( \left( \left( 1+\beta \right) {A}^{2}-16/3\,\rho _r \right) { c}+16/3\,\rho _r \right) \left( 1+\beta \right) {A}^{2}}+ \left( 3\,{A}^{2}\beta +3\,{A}^{2}-8 \,\rho _r \right) { c}+8\,\rho _r}{6{ c}\, \left( 1+\beta \right) }}\;, \end{aligned}$$
(176)
$$\begin{aligned}& \rho ^{2}_{T}=\frac{-3\,\sqrt{{A}^{2} \left( \left( {A}^{2}{\beta }^{2}+ \left( 2\,{A}^{2}+16/3\,\rho _r \right) \beta +{A}^{2}-16/3\,\rho _r \right) { c}-16/3\,\rho _r\, \left( \beta -1 \right) \right) \left( 1+\beta \right) ^{2}{ c}}}{6\left( \beta -1 \right) ^ {2}{ c}}\nonumber \\&\quad + \frac{\left( 3\,{A}^{2}{\beta }^{2}+ \left( 6\,{A}^{2}+8\,\rho _r \right) \beta +3\,{A}^{2}-8\,\rho _r \right) { c}-8\,\rho _r\, \left( \beta -1 \right) }{ 6\left( \beta -1 \right) ^ {2}{ c}}\;. \end{aligned}$$
(177)
In the same manner, by substituting \(f_1(T)\) and \(f_2(T)\) gravity models into Eq. (9) we calculate the pressure of the torsion fluid in MGCG as follows:
$$\begin{aligned}&p^{1}_{T} =\frac{-12\, \left( { c}-1 \right) \left( \beta +1/3 \right) \rho _r-3\,{A}^{2}{ c}\,\beta -3\,{A}^{2}{ c}}{ 6\left( 1+\beta \right) { c}}\nonumber \\&\quad + \frac{3\,\sqrt{{ c}\, \left( \left( \left( 1+\beta \right) {A}^{2}-16/ 3\,\rho _r \right) { c}+16/3\,\rho _r \right) \left( 1+\beta \right) {A}^{2}}}{ 6\left( 1+\beta \right) { c}} \;, \end{aligned}$$
(178)
$$\begin{aligned}&p^{2}_{T} = \frac{-12\, \left( { c}-1 \right) \left( \beta -1 \right) \left( \beta -1/3 \right) \rho _r-3\,{A}^{2}{ c}\,{\beta }^ {2}-6\,{A}^{2}{ c}\,\beta -3\,{A}^{2}{ c}}{ 6\left( \beta -1 \right) ^{2}{ c}}\nonumber \\&\quad +\frac{3\,\sqrt{{A}^{2} \left( \left( {A}^{2}{\beta }^{2}+ \left( 2\,{A}^{2}+16/3\,\rho _r \right) \beta +{A}^{2}-16/3\,\rho _r \right) { c}-16/3\,\rho _r\, \left( \beta -1 \right) \right) \left( 1+\beta \right) ^{2}{ c }}}{ 6\left( \beta -1 \right) ^{2}{ c}}\;. \end{aligned}$$
(179)
From the above energy density and the pressure terms of the fluid we obtain the equation of state parameter of the torsion fluid in MGCG model as follows:
$$\begin{aligned}&w^{1}_{T} =\frac{3\,\sqrt{{ c}\, \left( \left( \left( 1+\beta \right) {A}^{2}-16/3\,\rho _r \right) { c}+16/3\,\rho _r \right) \left( 1+ \beta \right) {A}^{2}}}{-3\,\sqrt{{ c}\, \left( \left( \left( 1+\beta \right) {A}^{2}-16/3\,\rho _r \right) { c}+16/3\,\rho _r \right) \left( 1+\beta \right) {A}^{2}}+ \left( 3\,{A}^{2}\beta +3\,{A}^{2}-8 \,\rho _r \right) { c}+8\,\rho _r} \nonumber \\&\quad +\frac{ \left( \left( -12\,\beta -4 \right) \rho _r-3\, \left( 1+\beta \right) {A}^{2} \right) { c}+ \left( 12\,\beta +4 \right) \rho _r}{-3\,\sqrt{{ c}\, \left( \left( \left( 1+\beta \right) {A}^{2}-16/3\,\rho _r \right) { c}+16/3\,\rho _r \right) \left( 1+\beta \right) {A}^{2}}+ \left( 3\,{A}^{2}\beta +3\,{A}^{2}-8 \,\rho _r \right) { c}+8\,\rho _r} \;, \end{aligned}$$
(180)
$$\begin{aligned}&w^{2}_{T} =\frac{3\,\sqrt{{A}^{2} \left( \left( {A}^{2}{\beta }^{2}+ \left( 2 \,{A}^{2}+16/3\,\rho _r \right) \beta +{A}^{2}-16/3\,\rho _r \right) { c}-16/3\,\rho _r\, \left( \beta -1 \right) \right) \left( 1+\beta \right) ^{2}{ c}}}{M_{1} } \nonumber \\&\quad +\frac{ \left( \left( -3\,{A}^{2}-12\,\rho _r \right) {\beta }^{2}+ \left( -6\,{A}^{2}+16\,\rho _r \right) \beta -3\,{A}^{2}-4\, \rho _r \right) { c}+12\,\rho _r\, \left( \beta -1 \right) \left( \beta -1/3 \right) }{M_{1} }\;, \end{aligned}$$
(181)
where
$$\begin{aligned}&M_{1}=-3\,\sqrt{{A}^{2} \left( \left( {A}^{2}{\beta }^{ 2}+ \left( 2\,{A}^{2}+16/3\,\rho _r \right) \beta +{A}^{2}-16/3\,\rho _r \right) { c}-16/3\,\rho _r\, \left( \beta -1 \right) \right) \left( 1+\beta \right) ^{2}{ c}}\nonumber \\&\quad + \left( 3\,{A}^{2}{\beta }^{2}+ \left( 6\,{A}^{2}+8\,\rho _r \right) \beta +3\,{A}^{2}-8\,\rho _r \right) { c}-8\,\rho _r\, \left( \beta -1 \right) . \end{aligned}$$
(182)
The plots in Fig. 13 show the effective equation of state parameter for radiation-torsion system for MGCG model. Then the fractional energy density of the torsion fluid express as follows:
$$\begin{aligned} \xi _{1}=\frac{-3\,\sqrt{{ c}\, \left( \left( \left( 1+\beta \right) {A}^{2}-16/3\,\rho _r \right) { c}+16/3\,\rho _r \right) \left( 1+\beta \right) {A}^{2}}+ \left( \left( 3+3\,\beta \right) {A }^{2}-8\,\rho _r \right) { c}+8\,\rho _r}{M_{2}}, \end{aligned}$$
(183)
where
$$\begin{aligned}&M_{2}=-3\,\sqrt{{A}^{2}{ c} \, \left( 1+\beta \right) \left( \left( \left( 1+\beta \right) {A}^ {2}-16/3\,\rho _{r,0} \right) { c}+16/3\,\rho _{r,0} \right) }\nonumber \\&\quad + \left( \left( 3+3\,\beta \right) {A}^{2}-8\,\rho _{r,0} \right) { c}+8\,\rho _r.\nonumber \\&\xi _{2}=\frac{ \left( -3\,{A}^{2}{ c}\,{\beta }^{2}+ \left( \left( -6 \,{A}^{2}-8\,\rho _r \right) { c}+8\,\rho _r \right) \beta + \left( -3 \,{A}^{2}+8\,\rho _r \right) { c}-8\,\rho _r \right) \left( 1+\beta \right) }{M_{4} }\nonumber \\&\quad \frac{+3\,\sqrt{{A}^{2} \left( \left( {A}^{2}{\beta }^{2}+ \left( 2\,{A}^{2}+16/3\,\rho _r \right) \beta +{A}^{2} -16/3\,\rho _r \right) { c}-16/3\,\rho _r\, \left( \beta -1 \right) \right) \left( 1+\beta \right) ^{2}{ c}}}{M_{4}}, \end{aligned}$$
(184)
where
$$\begin{aligned}&M_{4}= \left( \beta -1 \right) ^{2} \Big ( 3 \,\sqrt{ \left( 1+\beta \right) { c}\,{A}^{2} \left( \left( \left( 1+\beta \right) {A}^{2}-16/3\,\rho _{r,0} \right) { c}+16/3\, \rho _{r,0} \right) }\\&\quad -8\,\rho _{r,0} -3\,{A}^{2}{ c}\,\beta + \left( -3\,{A}^{2}+8\,\rho _{r,0} \right) { c}\Big ), \end{aligned}$$
and the ratio of effect energy density of the fluid
$$\begin{aligned} \chi _{1}=\frac{-3\,\sqrt{{ c}\, \left( \left( \left( 1+\beta \right) {A}^{2}-16/3\,\rho _r \right) { c}+16/3\,\rho _r \right) \left( 1+\beta \right) {A}^{2}}+ \left( \left( 3\,{A}^{2}+6\,\rho _r \right) \beta +3\,{A}^{2}-2\,\rho _r \right) { c}+8\,\rho _r}{M_{3}}, \end{aligned}$$
(185)
where
$$\begin{aligned}&M_{3}=-3\, \sqrt{{A}^{2}{ c}\, \left( 1+\beta \right) \left( \left( \left( 1+\beta \right) {A}^{2}-16/3\,\rho _{r,0} \right) { c}+16/3\, \rho _{r,0} \right) } \nonumber \\&\quad + \left( \left( 3\,{A}^{2}+6\,\rho _{r,0} \right) \beta +3\,{ A}^{2}-2\,\rho _{r,0} \right) { c}+8\,\rho _{r,0}, \nonumber \\&\chi _{2}=\frac{ \left( -3\,{ c}\, \left( {A}^{2}+2\,\rho _r \right) {\beta }^{2}+ \left( \left( -6\,{A}^{2}+4\,\rho _r \right) { c}+8\,\rho _r \right) \beta + \left( -3\,{A}^{2}+2\,\rho _r \right) { c}-8\,\rho _r \right) \left( 1+\beta \right) }{ M_{5}}\nonumber \\&\quad +\frac{+3\, \sqrt{{A}^{2} \left( \left( {A}^{2}{\beta }^{2}+ \left( 2\,{A}^{2}+16 /3\,\rho _r \right) \beta +{A}^{2}-16/3\,\rho _r \right) { c}-16/3\, \rho _r\, \left( \beta -1 \right) \right) \left( 1+\beta \right) ^{2}{ c}}}{M_{5}}, \end{aligned}$$
(186)
where
$$\begin{aligned}&M_{5}=\left( \Big ( \left( -3\,{A}^{2}-6\,\rho _{r,0} \right) \beta -3\,{A}^{2}+2\,\rho _{r,0} \right) { c}-8\,\rho _{r,0} \\&\quad +3\,\sqrt{ \left( 1+\beta \right) { c}\,{A}^ {2} \left( \left( \left( 1+\beta \right) {A}^{2}-16/3\,\rho _{r,0} \right) { c}+16/3\,\rho _{r,0} \right) }\Big ) \left( \beta -1 \right) ^{2}. \end{aligned}$$
The Eqs. (183) and (185) are presented on the left side of Fig. 14, and Eqs. (184) and (186) are presented on the right side of Fig. 14.
2.3.3 Dust-torsion system
As we indicated in the earlier in dust dominated Universe, the energy density of the pressure less fluid acts as a constant behind the exotic fluid from the early to late Universe [46]. In this limit, Eq. (168) will look like
$$\begin{aligned}&\frac{1}{(-f')^{(1+\alpha )}}\left[ -\frac{1}{2}(f-Tf')\right] \left[ (f'-1)\rho _d +\frac{1}{2}(f-Tf')\right] ^\alpha \nonumber \\&\quad =\beta \left[ -\frac{1}{f'}\left( (f'-1)\rho _d +\frac{1}{2}(f-Tf')\right) \right] ^{1+\alpha }-(1+\beta )A,\nonumber \\ \end{aligned}$$
(187)
For \(\alpha =-\frac{1}{2}\), the solutions as
$$\begin{aligned}&f_{1}(T)={ c}\,T-\frac{1}{{1+\beta }}\Big ({A}^{2}{ c}\,\beta +{A} ^{2}{ c}+2\,{ c}\,\beta \,\rho _d-2\,\beta \,\rho _d -\sqrt{{A}^{2 }{ c}\, \left( 1+\beta \right) \left( {A}^{2}{ c}\,\beta + {A}^{2}{ c}-4\,\rho _d\,{ c}+4\,\rho _d \right) }\Big ), \end{aligned}$$
(188)
$$\begin{aligned}&f_{2}(T)={ c}\,T-\frac{1}{(\beta -1)^{2}}\Big [{A}^{2}{ c}\,{\beta }^{ 2}+2\,{A}^{2}{ c}\,\beta +2\,{ c}\,{\beta }^{2}\rho _d +{A}^{2}{ c}-2\,{ c}\,\beta \,\rho _d-2\,{\beta }^{2}\rho _d +2\,\beta \,\rho _d\nonumber \\&\quad -\sqrt{{A}^{2}{ c}\, \left( 1+\beta \right) ^{2} \left( {A}^{2} { c}\,{\beta }^{2}+2\,{A}^{2}{ c}\,\beta +{A}^{2}{ c}+ 4\,{ c}\,\beta \,\rho _d-4\,\rho _d\,{ c}-4\,\beta \,\rho _d+4\,\rho _d \right) }~~\Big ], \end{aligned}$$
(189)
and the energy density of the fluid
$$\begin{aligned}&\rho ^{1}_{T}=\frac{ \left( -2\,\rho _d+ \left( 1+\beta \right) {A}^{2} \right) { c}-\sqrt{ \left( 1+\beta \right) { c}\, \left( \left( \left( 1+\beta \right) {A}^{2}-4\,\rho _d \right) { c}+4\,\rho _d \right) {A}^{2}}+2\,\rho _d}{ 2\left( 1+\beta \right) { c}}, \end{aligned}$$
(190)
$$\begin{aligned}&\rho ^{2}_{T}=\frac{-\sqrt{{ c}\, \left( 1+\beta \right) ^{2} \left( \left( {A}^{2}{\beta }^{2}+ \left( 2\,{A}^{2}+4\,\rho _d \right) \beta +{A }^{2}-4\,\rho _d \right) { c}-4\,\rho _d\, \left( \beta -1 \right) \right) {A}^{2}}}{ 2\left( \beta -1 \right) ^{2}{ c}}\nonumber \\&\quad +\frac{ \left( {A}^{2}{\beta }^{2}+ \left( 2\,{A}^{2}+2\, \rho _d \right) \beta +{A}^{2}-2\,\rho _d \right) { c}-2\,\beta \,\rho _d+2 \,\rho _d}{ 2\left( \beta -1 \right) ^{2}{ c}}\;. \end{aligned}$$
(191)
And the pressure of the fluid
$$\begin{aligned}&p^{1}_{T}=\frac{\sqrt{ \left( 1+\beta \right) { c}\, \left( \left( \left( 1+\beta \right) {A}^{2}-4\,\rho _d \right) { c}+4\, \rho _d \right) {A}^{2}}+ \left( \left( -{A}^{2}-4\,\rho _d \right) \beta -{ A}^{2}-2\,\rho _d \right) { c}+2\,\rho _d(1+2\beta )}{2{ c}\, \left( 1+\beta \right) }, \end{aligned}$$
(192)
$$\begin{aligned}&p^{2}_{T}=\frac{-4\, \left( \beta -1/2 \right) \left( \beta -1 \right) \left( { c}-1 \right) \rho _d-{A}^{2}{ c}\,{\beta }^{2}-2\,{A }^{2}{ c}\,\beta -{A}^{2}{ c}}{ 2\left( \beta -1 \right) ^{2 }{ c}}\nonumber \\&\quad +\frac{\sqrt{{ c}\, \left( 1+ \beta \right) ^{2} \left( \left( {A}^{2}{\beta }^{2}+ \left( 2\,{A}^{2 }+4\,\rho _d \right) \beta +{A}^{2}-4\,\rho _d \right) { c}-4\,\rho _d\, \left( \beta -1 \right) \right) {A}^{2}}}{ 2\left( \beta -1 \right) ^{2 }{ c}}. \end{aligned}$$
(193)
The corresponding equation of state parameters are give as follows:
$$\begin{aligned}&w^{1}_T ={\frac{\sqrt{ \left( 1+\beta \right) { c}\, \left( \left( \left( 1+\beta \right) {A}^{2}-4\,\rho _d \right) { c}+4\,\rho _d \right) {A}^{2}}+ \left( \left( -4\,\beta -2 \right) \rho _d-{A}^{2} \beta -{A}^{2} \right) { c}+ \left( 4\,\beta +2 \right) \rho _d}{- \sqrt{ \left( 1+\beta \right) { c}\, \left( \left( \left( 1+ \beta \right) {A}^{2}-4\,\rho _d \right) { c}+4\,\rho _d \right) {A}^{ 2}}+ \left( {A}^{2}\beta +{A}^{2}-2\,\rho _d \right) { c}+2\,\rho _d}}, \end{aligned}$$
(194)
$$\begin{aligned}&w^{2}_T = \frac{4\, \left( \beta -1/2 \right) \left( \beta -1 \right) \left( { c}-1 \right) \rho _d+{A}^{2}{ c}\,{\beta }^{2}+2\,{A}^{2}{ c}\,\beta +{A}^{2}{ c}}{M_{6}}- \nonumber \\&\quad \frac{\sqrt{{ c}\, \left( 1+\beta \right) ^{2} \left( \left( {A}^{2}{\beta }^{2}+ \left( 2\,{A}^{2}+4\, \rho _d \right) \beta +{A}^{2}-4\,\rho _d \right) { c}-4\,\rho _d\, \left( \beta -1 \right) \right) {A}^{2}}}{M_{6}}, \end{aligned}$$
(195)
where
$$\begin{aligned}&M_{6}=-2\, \left( \beta -1 \right) \left( { c}-1 \right) \rho _d-{A}^{2}{ c}\,{\beta }^ {2}-2\,{A}^{2}{ c}\,\beta -{A}^{2}{ c}\\&\quad +\sqrt{{ c}\, \left( 1+\beta \right) ^{2} \left( \left( {A}^{2}{\beta }^{2}+ \left( 2\,{A}^{2}+4\,\rho _d \right) \beta +{A}^{2}-4\,\rho _d \right) { c}-4\,\rho _d\, \left( \beta -1 \right) \right) {A}^{2}} \end{aligned}$$
Figure 15 shows the effective equation of state parameter for dust-torsion system for MGCG model. The ratio of the energy density in torsion fluid expressed as follows:
$$\begin{aligned} \xi _{1}= & {} {\frac{-3\,\sqrt{ \left( 1+\beta \right) { c}\, \left\{ \left[ \left( 1+\beta \right) {A}^{2}-4\,\rho _d \right] { c}+4\, \rho _d \right\} {A}^{2}}+ \left[ \left( 3\,\beta +3 \right) {A}^{2}-6\, \rho _d \right] { c}+6\,\rho _d}{-3\,\sqrt{{A}^{2}{ c}\, \left( 1+\beta \right) \left\{ \left[ ( 1+\beta ) {A}^{2 }-\frac{16}{3}\rho _{d,0} \right] { c}+\frac{16}{3}\rho _{d,0} \right\} }+ \left[ ( 3\,\beta +3) {A}^{2}-8\,\rho _{d,0} \right] { c}+8\,\rho _d}}, \end{aligned}$$
(196)
$$\begin{aligned} \xi _{2}= & {} \frac{ \Big [ -\sqrt{{ c}\, \left( 1+\beta \right) ^{2} \left( \left( {A}^{2}{\beta }^{2}+ \left( 2\,{A}^{2}+4\,\rho _d \right) \beta +{A}^{2}-4\,\rho _d \right) { c}-4\,\rho _d\, \left( \beta -1 \right) \right) {A}^{2}}}{M_{8}}\nonumber \\&+ \frac{\left( {A}^{2}{\beta }^{2}+ \left( 2\,{A}^{ 2}+2\,\rho _d \right) \beta +{A}^{2}-2\,\rho _d \right) { c}-2\,\rho _d\, \left( \beta -1 \right) \Big ] \left( 1+\beta \right) }{ M_{8}}, \end{aligned}$$
(197)
where
$$\begin{aligned}&M_{8}=\Big [ - \sqrt{ \left( 1+\beta \right) { c}\,{A}^{2} \left\{ \left[ ( 1+\beta ) {A}^{2}-16/3\,\rho _{d,0} \right] { c}+16/3\, \rho _{d,0} \right\} } \\&\quad + \left( {A}^{2}\beta +{A}^{2}-8/3\,\rho _{d,0} \right) { c}+8/3\,\rho _{d,0} \Big ] \left( \beta -1 \right) ^{2}. \end{aligned}$$
The ratio of the effective energy density of the fluid expressed as follows
$$\begin{aligned} \chi _{1}=\frac{-3\,\sqrt{ \left( 1+\beta \right) { c}\, \left\{ \left[ \left( 1+\beta \right) {A}^{2}-4\,\rho _d \right] { c}+4\, \rho _d \right\} {A}^{2}}+ \left( \left( 3\,{A}^{2}+6\,\rho _d \right) \beta +3\,{A}^{2} \right) { c}+6\,\rho _d}{M_{7}}, \end{aligned}$$
(198)
where
$$\begin{aligned} M_{7}= & {} -3\,\sqrt{{A}^{2}{ c}\, \left( 1+\beta \right) \left\{ \left[ \left( 1+\beta \right) {A}^{2 }-16/3\,\rho _{d,0} \right] { c}+16/3\,\rho _{d,0} \right\} } + \left( \left( 3\,{A}^{2}+6\,\rho _{d,0} \right) \beta +3\,{A}^{2}-2\,\rho _{d,0} \right) { c}+8\,\rho _{d,0}\nonumber \\ \chi _{2}= & {} \frac{3}{ M_{9} }\Big \{\Big [ - \left( {A}^{2}+2\,\rho _d \right) { c}\,{\beta }^{2}+ \left( \left( -2\,{A}^{2}+2\,\rho _d \right) { c}+2\,\rho _d \right) \beta -{A}^{2}{ c}\nonumber \\&+\sqrt{{ c}\, \left( 1+\beta \right) ^{2} \left( \left( {A}^{2}{\beta }^{2}+ \left( 2\,{A}^{2}+4\, \rho _d \right) \beta +{A}^{2}-4\,\rho _d \right) { c}-4\,\rho _d\, \left( \beta -1 \right) \right) {A}^{2}}-2\,\rho _d \Big ] \left( 1+ \beta \right) \Big \}, \end{aligned}$$
(199)
where
$$\begin{aligned} M_{9}= & {} \left( \beta -1 \right) ^{2} \Big [ \left( \left( -3 \,{A}^{2}-6\,\rho _{d,0} \right) \beta -3\,{A}^{2}+2\,\rho _{d,0} \right) { c }\\&+3\,\sqrt{ \left( 1+\beta \right) { c}\,{A}^{2} \left( \left( \left( 1+\beta \right) {A}^{2}-16/3\,\rho _{d,0} \right) { c} +16/3\,\rho _{d,0} \right) }-8\,\rho _{d,0} \Big ]. \end{aligned}$$
The Eqs. (196) and (198) are presented on the left side of Fig. 16, and Eqs. (197) and (199) are presented on the right side of Fig. 16.
2.3.4 Stiff matter-torsion system
Here also we consider the stiff fluid as an exotic fluid in MGCG and the general expression of Eq. (168) and we obtain
$$\begin{aligned}&\frac{1}{(-f')^{(1+\alpha )}}\left[ (f'-1)w\rho _s-\frac{1}{2}(f-Tf')\right] \nonumber \\&\qquad \left[ (f'-1)\rho _d +\frac{1}{2}(f-Tf')\right] ^\alpha \nonumber \\&\quad =\beta \left[ -\frac{1}{f'}\left( (f'-1)\rho _s +\frac{1}{2}(f-Tf')\right) \right] ^{1+\alpha }\nonumber \\&\qquad -(1+\beta )A, \end{aligned}$$
(200)
with the solutions of
$$\begin{aligned} f_1\left( T \right)= & {} { c}\,T- {\frac{{A}^{2}{ c}\, \beta +{A} ^{2}{ c}+2\,{ c}\,\beta \,\rho _s-2\,\rho _s\,{ c} -2\,\beta \,\rho _s-\sqrt{{A}^{2}{ c}\, \left( 1+\beta \right) \left( {A}^{ 2}{ c}\,\beta +{A}^{2}{ c}-8\,\rho _s\,{ c}+8\, \rho _s \right) }+2\,\rho _s}{1+\beta }} \end{aligned}$$
(201)
$$\begin{aligned} f_2\left( T \right)= & {} { c}\,T-{\frac{{A}^{2}{ c}\, \beta +{A}^{2}{ c}+2\,{ c}\,\beta \,\rho _s-2\,\rho _s\, { c} -2\,\beta \,\rho _s}{\beta -1}}\nonumber \\&{\frac{ -\sqrt{{A}^{2}{ c}\, \left( {A}^{2}{ c}\,{ \beta }^{2}+2\,{A}^{2}{ c}\,\beta +{A}^{2}{ c}+8\, { c} \,\beta \,\rho _s-8\,\rho _s\,{ c}-8\,\beta \,\rho _s+8\,\rho _s \right) }+2\, \rho _s }{\beta -1}}. \end{aligned}$$
(202)
We reconstruct the energy density by substituting \(f_1(T)\) and \(f_{2}(T)\) into Eq. (7) and we obtain
$$\begin{aligned}&\rho ^{T}_{1} = \,{\frac{ \left( \left( 1+\beta \right) {A}^{2}-4\,\rho _s \right) { c}-\sqrt{ \left( \left( \left( 1+\beta \right) {A}^ {2}-8\, \rho _s \right) { c}+8\,\rho _s \right) {A}^{2}{ c}\, \left( 1+ \beta \right) }+4\,\rho _s}{2 \left( 1+\beta \right) { c}}} , \end{aligned}$$
(203)
$$\begin{aligned}&\rho ^2_T = \frac{{A}^{2 }{ c}\,{\beta }^{2}+ \left( \left( 2\,{A}^{2}+4\,\rho _s \right) { c}-4\,\rho _s \right) \beta + \left( {A}^{2}-4\,\rho _s \right) { c}+4\,\rho _s}{2\left( \beta -1 \right) ^{2}{ c}}\nonumber \\&\quad + \,{\frac{ \left( -\beta -1 \right) \sqrt{{ c}\,{A}^ {2} \left( { c}\, \left( 1+\beta \right) ^{2}{A}^{2}+8\, \rho _s\, \left( \beta -1 \right) \left( { c}-1 \right) \right) } }{ 2\left( \beta -1 \right) ^{2}{ c}}} \;. \end{aligned}$$
(204)
Here also we calculate the pressure of the torsion fluid by substituting \(f_1(T)\) and \(f_{2}(T)\) into Eq. (9) and we obtain
$$\begin{aligned}&p^1_T =-\frac{ \rho _s\, \left( { c}-1 \right) }{2c(1+ \beta )} \Big [ {A}^{2}{ c}\,\beta +{A}^{2}{ c}+2\,{ c}\, \beta \,\rho _s-2\,{ c}\,\rho _s-2\,\beta \,\rho _s -\sqrt{{A}^{2} { c }\, \left( 1+\beta \right) \left( {A}^{2}{ c}\,\beta +{A} ^{2}{ c}-8\,{ c}\,\rho _s+8\,\rho _s \right) }+2c\,\rho _s\Big ],\\&p_T^2 = \,{\frac{ \left( 1+\beta \right) \sqrt{{ c}\, \left( { c}\, \left( 1+\beta \right) ^{2}{A}^{2}+8\,\rho \, \left( \beta -1 \right) \left( { c}-1 \right) \right) {A}^{2}}+ \left( \left( -{A}^{2}-4\,\rho \right) { c}+4\,\rho \right) {\beta }^{2 }+ \left( \left( -2\,{A}^{2}+4\,\rho \right) { c}-4\, \rho \right) \beta -{A}^{2}{ c}}{ 2\left( \beta -1 \right) ^{2} { c}}}\;. \end{aligned}$$
2.3.5 Radiation-dust-torsion system
Here is the general expression of radiation-dust-torsion system as an exotic fluid in MGCG model
$$\begin{aligned}&\frac{1}{(-f')^{(1+\alpha )}}\left[ (f'-1)p_m -\frac{1}{2}(f-Tf')\right] \nonumber \\&\qquad \left[ (f'-1)\rho _m +\frac{1}{2}(f-Tf')\right] ^\alpha \nonumber \\&\quad =\beta \left[ -\frac{1}{f'}\left( (f'-1)\rho _m +\frac{1}{2}(f-Tf')\right) \right] ^{1+\alpha }\nonumber \\&\qquad -(1+\beta )A, \end{aligned}$$
(205)
with solutions given as
$$\begin{aligned}&f_{1}(T) = { c}\,T-\frac{1}{(\beta -1)^{ 2}}\Big [{A}^{2}{ c}\,{\beta }^{ 2}+2\,{A}^{2}{ c}\,\beta +2\,{ c}\,{\beta }^{2}\rho \nonumber \\&\quad +{A}^{2}{ c}+2\,{ c}\,\beta \,p-2\,{ c}\,\beta \,\rho \nonumber \\&\quad -2\,\rho \, {\beta }^{2}-2\,{ c}\,p-2\,\beta \,p+2\,\beta \,\rho \nonumber \\&\quad -\Big ( {A}^{2}{ c}\, \left( 1+\beta \right) ^{2} \big ( {A}^{2}{ c}\,{ \beta }^{2}+2\,{A}^{2}{ c}\,\beta +{A}^{2}{ c}\nonumber \\&\quad +4\,{ c}\,\beta \,p+ 4\,{ c}\,\beta \,\rho -4\,{ c}\,p-4\,{ c}\, \rho -4\,\beta \,p\nonumber \\&\quad -4\,\beta \,\rho +4\,p+4\,\rho \big ) \Big )^{\frac{1}{2}}+2\,p\Big ], \end{aligned}$$
(206)
$$\begin{aligned}&f_{2}(T) = { c}\,T-\frac{1}{1+\beta }\Big [{A}^{2}{ c}\,\beta +{A} ^{2}{ c}\nonumber \\&\quad +2\,{ c}\,\beta \,\rho -2\,{ c}\,p-2\,\beta \, \rho \nonumber \\&\quad -\Big ({A}^{2}{ c}\, \left( 1+\beta \right) \left( {A}^{2} { c}\,\beta +{A}^{2}{ c}-4\,{ c}\,p\right. \nonumber \\&\quad -\left. 4\,{ c}\, \rho +4\,p+4\,\rho \right) \Big )^{\frac{1}{2}}+2\,p\Big ]\;. \end{aligned}$$
(207)
From this constructed \(f_1(T)\) and \(f_2(T)\) gravity model we can reconstruct the energy density of the torsion fluid in the non-interacting fluid. By substituting \(f_1(T)\) and \(f_2(T)\) into Eq. (7), we obtain
$$\begin{aligned}&\rho ^{1}_{T}=\frac{1}{ 2\left( \beta -1 \right) ^{2}{ c}}\Big [-\Big ({ c}\,{A}^{2} \big ( \left( {A}^{2}{\beta } ^{2}\right. +\left. \left( 2\,{A}^{2}+4\,p+4\,\rho \right) \beta +{A}^{2}-4\,p-4\, \rho \right) { c}\nonumber \\&\quad -4\, \left( \beta -1 \right) \left( p+\rho \right) \big ) \left( 1+\beta \right) ^{2}\Big )^{\frac{1}{2}}+ \big ( {A}^{2}{\beta } ^{2} +\left( 2\,{A}^{2}+2\,p+2\,\rho \right) \beta +{A}^{2}-2\,p-2\, \rho \big ) { c}\nonumber \\&\quad + \left( -2\,p-2\,\rho \right) \beta +2\,p+2\, \rho \Big ] \end{aligned}$$
(208)
$$\begin{aligned}&\rho ^{2}_{T}=\frac{1 }{2{ c}\, \left( 1+ \beta \right) }\Big [-\sqrt{{ c}\, \left\{ \left[ \left( 1+\beta \right) {A}^{2}-4\,p-4\,\rho \right] { c}+4\,p+4\,\rho \right\} {A}^{2} \left( 1+\beta \right) }\nonumber \\&\quad +\left( -2\,\rho + \left( 1+\beta \right) {A}^{2}-2\,p \right) { c}+2\,p+2\,\rho \Big ], \end{aligned}$$
(209)
and by substituting \(f_1(T)\) and \(f_2(T)\) into Eq. (9), we obtain pressure of the fluid as follows:
$$\begin{aligned} p^{1}_{T}= & {} \frac{1}{ 2\left( \beta -1 \right) ^{2}{ c}}\Big [-{A}^{2}{ c}\, \left( 1+\beta \right) ^{2}-2\,\beta \, \left( \beta -1 \right) \left( p+\rho \right) { c} +2\,\beta \, \left( \beta -1 \right) \rho +2\,p{\beta }^{2}-2\,\beta \,p\nonumber \\&+\sqrt{{ c}\,{A}^{2} \left( \left( {A}^{2}{\beta }^{2}+ \left( 2\,{A}^{2}+4 \,p+4\,\rho \right) \beta +{A}^{2}-4\,p-4\,\rho \right) { c}-4\, \left( \beta -1 \right) \left( p+\rho \right) \right) \left( 1+ \beta \right) ^{2}}\Big ], \end{aligned}$$
(210)
$$\begin{aligned} p^{2}_{T}= & {} \frac{1}{2{ c}\, \left( 1+\beta \right) }\Big [\sqrt{{ c}\, \left\{ \left[ \left( 1+\beta \right) {A}^{2}-4\,p-4\,\rho \right] { c}+4\,p+4\,\rho \right\} {A}^{2} \left( 1+\beta \right) } \nonumber \\&+ \left( \left( -{A}^{2}-2\,p-2\,\rho \right) { c}+2\,p+2\,\rho \right) \beta -{A}^{2}{ c}\Big ]. \end{aligned}$$
(211)
The equation of state parameter for torsion fluid become as follows:
$$\begin{aligned} \begin{aligned} w^{1}_{T}&= \frac{\sqrt{{ c}\,{A}^{2} \left( \left( {A}^{2}{\beta }^{2}+ \left( 2\,{A}^{2}+4\,p+4\,\rho \right) \beta +{A}^{2}-4\,p-4\,\rho \right) { c}-4\, \left( \beta -1 \right) \left( p+\rho \right) \right) \left( 1+\beta \right) ^{2}}}{M_{10}}\\&\quad + \frac{\left( \left( -{A}^{2}-2\,p-2 \,\rho \right) { c}+2\,p+2\,\rho \right) {\beta }^{2}+ \left( \left( -2\,{A}^{2}+2\,p+2\,\rho \right) { c}-2\,p-2\,\rho \right) \beta -{A}^{2}{ c}}{M_{10}},\\ w^{2}_{T}&=\frac{1}{M_{11}}\Big [\sqrt{{ c}\, \left\{ \left[ \left( 1+\beta \right) {A} ^{2}-4\,p-4\,\rho \right] { c}+4\,p+4\,\rho \right\} {A}^{2} \left( 1+\beta \right) }\\&\quad + \left( \left( -{A}^{2}-2\,p-2\,\rho \right) \beta -{A}^{2} \right) { c}+ \left( 2\,\rho +2\,p \right) \beta \Big ], \end{aligned} \end{aligned}$$
(212)
$$\begin{aligned}&\hbox {where}\quad M_{10}= {A}^{2}{ c}\,{\beta }^{2}+ \left( \left( 2\,{A}^{2}+2\,p+2\, \rho \right) { c}-2\,p-2\,\rho \right) \beta + \left( {A}^{2}-2\, p-2\,\rho \right) { c}+2\,p+2\,\rho \\&-\sqrt{{c}\,{A}^{2} \left\{ \left[ {A}^{2}{\beta }^{2}+ \left( 2\,{A}^{2}+4\,p+4\,\rho \right) \beta +{A}^{2}-4\,p-4\,\rho \right] { c}-4\, \left( \beta -1 \right) \left( p+\rho \right] \right\} \left( 1+\beta \right) ^{2}}\\&\hbox {and} \quad M_{11}= \left( {A}^{2}\beta +{A}^{2}-2\,p-2\, \rho \right) { c}+2\,p+2\,\rho -\sqrt{{ c}\, \left\{ \left[ \left( 1+\beta \right) {A}^{2}-4\,p-4\,\rho \right] { c}+4\,p+4\,\rho \right\} {A}^{2} \left( 1+\beta \right) }. \end{aligned}$$
The numerical results of these equation state parameters is presented in Fig. 17 for MGCG model in radiation-dust-torsion system. The the growth factor parameter of energy density of torsion fluid
$$\begin{aligned} \begin{aligned} \xi _{1}&= \frac{ \left( 1+\beta \right) }{ M_{12} }\Big [ \left( {A}^{2}{\beta } ^{2}+ \left( 2\,{A}^{2}+2\,p+2\,\rho \right) \beta +{A}^{2}-2\,p-2\, \rho \right) { c}-2\, \left( \beta -1 \right) \left( p+\rho \right) \\&-\sqrt{{ c}\,{A}^{2} \left\{ \left[ {A}^{2}{ \beta }^{2}+ \left( 2\,{A}^{2}+4\,p+4\,\rho \right) \beta +{A}^{2}-4\,p- 4\,\rho \right] { c}-4\, \left( \beta -1 \right) \left( p+\rho \right) \right\} \left( 1+\beta \right) ^{2}}\Big ], \end{aligned} \end{aligned}$$
(213)
$$\hbox {where} \,M_{12}=\left( \beta -1 \right) ^{ 2} \Big [ -\sqrt{ \left( 1+\beta \right) { c}\,{A}^{2} \left( \left( \left( 1+\beta \right) {A}^{2}-16/3\,\rho _0 \right) { c} +16/3\,\rho _0 \right) }+ \left( {A}^{2}\beta +{A}^{2}-8/3\,\rho _0 \right) { c}+8/3\,\rho _0 \Big ]$$
and
$$\begin{aligned} \begin{aligned} \xi _{2}&= \frac{1}{M_{14}}\Big [-3\,\sqrt{{ c}\, \left\{ \left[ \left( 1+\beta \right) {A}^{2}-4\,p-4\,\rho \right] { c}+4\,p+4\,\rho \right\} {A}^{2} \left( 1+\beta \right) } + \left( \left( 3\,\beta +3 \right) {A }^{2}-6\,p-6\,\rho \right) { c}+6\,p+6\,\rho \Big ], \end{aligned} \end{aligned}$$
(214)
where \(M_{14}=-3\,\sqrt{ \left( 1+\beta \right) { c}\,{A}^{2} \left\{ \left[ \left( 1+ \beta \right) {A}^{2}-16/3\,\rho _0 \right] { c}+16/3\,\rho _0 \right\} }+ \left( \left( 3\right. \right. \left. \left. \beta +3 \right) {A}^{2}-8\,\rho _0 \right) { c}+8\,\rho _0.\) And the growth factor parameters for effective fluid become:
$$\begin{aligned} \begin{aligned} \chi _{1}&=\frac{3}{M_{13}}\Big [\Big ( - \left( {A}^{2}+2\,\rho \right) { c}\,{\beta }^{2}+ \left( \left( -2\,{A}^{2}-2\,p+2\,\rho \right) { c}+2\,p +2\,\rho \right) \beta + \left( -{A}^{2}+2\,p \right) {c}\\&\quad +\sqrt{{ c}\,{A}^{2} \left\{ \left[ {A}^{2}{\beta }^{2}+ \left( 2\,{A}^ {2}+4\,p+4\,\rho \right) \beta +{A}^{2}-4\,p-4\,\rho \right] { c} -4\, \left( \beta -1 \right) \left( p+\rho \right) \right\} \left( 1+ \beta \right) ^{2}}\\&\quad -2\,p-2\,\rho \Big ) \left( 1+\beta \right) \Big ], \end{aligned} \end{aligned}$$
(215)
where \(M_{13}= \left( \beta -1 \right) ^{2} \Big [ \left( \left( -3\,{A}^{2}-6\, \rho _0 \right) \beta -3\,{A}^{2}+2\,\rho _0 \right) { c}+3\,\sqrt{ \left( 1+\beta \right) { c}\,{A}^{2} \left( \left( \left( 1+ \beta \right) {A}^{2}-16/3\,\rho _0 \right) { c}+16/3\,\rho _0 \right) }-8\,\rho _0 \Big ],\) and
$$\begin{aligned} \begin{aligned} \chi _{2}&=\frac{1}{M_{15}}\Big [-3\,\sqrt{{ c}\, \left\{ \left[ \left( 1+\beta \right) {A}^{2}-4\,p-4\,\rho \right] { c}+4\,p+4\,\rho \right\} {A}^{2} \left( 1+\beta \right) }\\&\quad + \bigg ( \left( 3\,{A}^{2}+6\,\rho \right) \beta +3\,{A}^{2}-6\,p \bigg ) { c}+6\,p+6\,\rho \Big ], \end{aligned} \end{aligned}$$
(216)
where \(M_{15}=-3 \sqrt{ \left( 1+\beta \right) { c}\,{A}^{2} \left\{ \left[ \left( 1+\beta \right) {A}^{2}-16/3\,\rho _0 \right] { c}+16/3\, \rho _0 \right\} } + \left( \left( 3\,{A}^{2}+6\,\rho _0 \right) \beta +3\,{ A}^{2}-2\,\rho _0 \right) { c}+8\,\rho _0\). The Eqs. (213) and (215) are presented on the left side of Fig. 18, and Eqs. (214) and (216) are presented on the right side of Fig. 18.